The galaxy presents a generally elliptical morphology, although there is some evidence of a faint disk-like structure. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population and potentially an active galactic nucleus, however the color appears redder. The light falls off gradually, and the colors get bluer further from the center. There is a slight asymmetry in the outskirts, possibly indicating minor tidal interactions or past merger events. The overall color index suggests an intermediate age stellar population, with ongoing, but not intensive, star formation. The galaxy appears relatively isolated, with no immediately apparent major companion galaxies.