The galaxy appears to be in the process of a merger or experiencing significant tidal interactions. The main body of the galaxy presents a relatively smooth, elliptical morphology, with a bright central nucleus. A plume-like extension is visible extending from the main body, suggesting a significant gravitational disturbance. This structure displays a bluer hue than the main galactic body, indicating a possible region of active star formation triggered by the interaction. There is noticeable asymmetry in the outer regions, which further supports the merger scenario. Overall, the galaxy exhibits a disturbed morphology indicative of ongoing interaction with another galaxy or tidal disruption.
