The galaxy appears to be in the late stages of a merger. There are two distinct nuclei visible. The larger nucleus shows a more diffuse, smooth appearance with a bluish-white hue, suggestive of an older stellar population and potentially ongoing star formation. The smaller nucleus, slightly offset, exhibits a more yellowish-orange color, possibly indicating a higher proportion of older stars or dust obscuration. There is faint tidal debris visible extending from the main body of the galaxy, hinting at gravitational disturbances related to the interaction. The overall shape is irregular, with the major axis elongated. The system is neither purely elliptical nor a well-defined spiral. The presence of two nuclei and disturbed morphology supports the assessment of an ongoing merger.
