The galaxy presents as a centrally concentrated, fairly regular elliptical galaxy with a smooth light profile. It exhibits a high degree of roundness. The light is generally homogenous across the visible surface, with no obvious features like spiral arms, dust lanes, or strong tidal disturbances present. The galaxy's color appears to be slightly redder, indicative of an older stellar population and lower ongoing star formation. There is no evidence of a major merger event or significant interactions with neighboring galaxies based on the smooth and undisturbed appearance. The galaxy is a relatively luminous object, suggestive of a substantial stellar mass.
