The galaxy appears to be undergoing a significant interaction, possibly a merger event. There are noticeable disturbances in its morphology, including a prominent tidal tail extending outward. The central region shows signs of disruption, and there may be multiple nuclei or areas of concentrated luminosity. The overall color profile suggests a mix of stellar populations, with regions of bluer light indicative of ongoing star formation and redder areas possibly containing older stars. The galaxy does not appear to have a defined disk structure and presents an irregular shape.
