The Hubble Space Telescope previously spotted a distant galaxy that shows visible signs of a collision and merger with its galactic neighbour. According to the European Space Agency (ESA), the galaxy's violent past led to the formation of new stars.

The cosmic structure feature in the photo has been identified as the galaxy NGC 7714. It is located in the Pisces constellation and is about 100 million light-years from Earth's neighbourhood.

NGC 7714's Deformed Shape

NGC 7714
The NASA/ESA Hubble Space Telescope has captured this striking view of spiral galaxy NGC 7714. This galaxy has drifted too close to another nearby galaxy and the dramatic interaction has twisted its spiral arms out of shape, dragged streams of material out into space, and triggered bright bursts of star formation. ESA/NASA/Hubble

Like Milky Way, NGC 7714 is also classified as a spiral galaxy, which is characterized by its swirling spindly arms. Although NGC 7714 is technically a spiral galaxy, it looks very different from Milky Way due to its disfigured appearance. As explained by the ESA, NGC 7714 was disfigured following a collision with a smaller neighbouring galaxy known as NGC 7715. According to the agency, these two galaxies drifted close to one another millions of years ago.

As the galaxies collided into one another, the smaller NGC 7715 began to merge with NGC 7714, causing disruptions in the latter's arms. "The culprit is a smaller companion named NGC 7715, which lies just out of the frame of this image — but is visible in the wider-field DSS image," ESA explained. "The two galaxies [1] drifted too close together between 100 and 200 million years ago, and began to drag at and disrupt one another's structure and shape."

Effect Of Merger On NGC 7714

The collision and merger created a new feature on NGC 7714, which is a tail-like structure extending into NGC 7715. This cosmic bridge serves as a funnel that delivers stellar materials from the smaller galaxy into its larger neighbour. The influx of materials such as gas and dust led to a burst of new star formations within NGC 7714. According to the ESA, most of the newborn stars within the galaxy can be found near its bright central region.

"A ring and two long tails of stars have emerged from NGC 7714, creating a bridge between the two galaxies," ESA stated. "This bridge acts as a pipeline, funneling material from NGC 7715 towards its larger companion and feeding bursts of star formation. Most of the star-forming activity is concentrated at the bright galactic centre, although the whole galaxy is sparking new stars."