The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually fades into an outer halo. The overall color appears to be redder in the visual bands, suggesting a population of older stars. The galaxy appears to be isolated, showing no obvious signs of tidal disturbances or interactions with other galaxies in its immediate vicinity. There is no discernible dust lane or prominent spiral arm structure. It looks to be a massive galaxy with suppressed star formation.
