This galaxy appears to be undergoing a significant merger event. Its morphology is highly disturbed, with a pronounced tidal tail emanating from the main body. The central region exhibits a bright, concentrated core suggesting an active galactic nucleus (AGN) or a recent burst of star formation. The overall color is relatively red, suggesting an older stellar population and a possible lack of ongoing star formation in the extended regions. The main body appears to be comprised of two distinct components, indicating the possible ongoing collision and eventual merging of two separate galaxies. Evidence of significant dust lanes or structures obscuring parts of the galaxy are not readily apparent.
