This galaxy exhibits a merging morphology, characterized by two distinct, bright nuclei suggesting ongoing or recent interaction. The primary component appears ellipsoidal, with a smooth, diffuse halo. The secondary nucleus is smaller and less defined, potentially a disrupted galaxy core or a region of intense star formation triggered by the merger. The overall color is predominantly redder, indicating a population of older stars or significant dust obscuration. Faint tidal features or extended stellar streams are suspected, though resolution limitations make precise delineation difficult. The galaxy is moderately sized, exhibiting significant luminosity.
