The galaxy presents as a generally smooth, centrally concentrated object with a slight elongation. The morphology is not perfectly elliptical, appearing somewhat disturbed, possibly due to a past or ongoing interaction. The core exhibits a yellow-white hue, suggesting a population of older stars. Above and to the right of the main body, there is what appears to be a pair of distinct but nearby, reddish luminous regions. These areas could potentially be separate interacting galaxies, star-forming regions heavily obscured by dust, or tidal features resulting from a merger. If these are galaxies, they appear to be at different stages of merging. The overall color suggests a redshifted object with a moderate to high stellar mass and potentially moderate star formation.
