The galaxy presents as a system dominated by a single, large elliptical galaxy, appearing relatively smooth in texture with minimal discernible substructure. The light distribution suggests a centrally concentrated spheroid, with a gradual decrease in luminosity outwards. The overall color index leans toward the redder end of the spectrum, indicative of an older stellar population and/or significant dust obscuration. There is a smaller galaxy relatively close to the primary galaxy, which could mean the galaxies are currently undergoing some sort of interaction. The red color of the galaxy suggests that there is minimal ongoing star formation within the galaxy.
