This galaxy exhibits a complex morphology, suggestive of an ongoing or recent merger event. The primary component appears relatively smooth and elliptical in shape, indicating an older stellar population. However, there is a distinct tidal tail or stream of material extending outwards, indicating gravitational disturbance. This stream displays a redder color, implying potentially older stars or dust obscuration. There are also multiple areas of high brightness, potentially areas of high star formation, or the nuclei of the merger remnants. The system is fairly compact. Overall, the galaxy presents characteristics of a dynamically disturbed system, likely experiencing tidal interactions that have disrupted its original structure.
