The galaxy presents as a moderately bright, diffuse object. It appears elliptical in shape, displaying a concentrated central bulge surrounded by a more extended, fainter halo. The color profile suggests a bias towards redder wavelengths, particularly within the central region, potentially indicative of an older stellar population. There is a faint blue coloring in the outer regions, suggestive of possible star formation but it is faint. The galaxy appears relatively undisturbed, without obvious signs of a major merger event. Slight asymmetry is observed in the halo, possibly reflecting minor tidal interactions or internal dynamical processes. The smooth light distribution supports the classification as a relatively quiescent system.
