This galaxy appears to have a disturbed morphology, potentially indicative of an ongoing or recent merger event. The primary body of the galaxy exhibits a smooth, elliptical-like appearance with a concentration of light towards its center, suggesting an older stellar population. There is a secondary, less-defined structure extending from the main body of the galaxy. This appendage shows a bluer color, hinting at more recent star formation within this region. The overall color of the galaxy is yellowish, which is likely due to the presence of older stars. There are suggestions of tidal tails or other debris extending outwards, further supporting the hypothesis of an interaction with another galaxy.
