The galaxy appears as a somewhat rounded, concentrated light source with a smooth overall profile. Its color is predominantly yellowish-orange, which could indicate an older stellar population. There is no discernible spiral structure or significant dust lane obscuration. The galaxy exhibits a slight elongation, deviating somewhat from a perfectly circular shape. There appears to be a small hint of possible tidal disturbances, but the smoothness of the primary light profile suggests a galaxy that has not undergone recent major mergers. The concentrated light indicates this galaxy is an early type galaxy with a red shift of approximately 0.3.