The galaxy presents a generally smooth, elliptical morphology. The core exhibits a concentrated luminosity with a reddish-yellow hue, suggestive of an older stellar population. A fainter, more diffuse halo of bluish light surrounds the central region, implying the presence of some younger, hotter stars, and possibly some ongoing star formation, although at a low rate. The overall structure appears largely undisturbed, lacking prominent spiral arms or tidal features. The galaxy is somewhat rounded in shape and exhibits no obvious signs of a major merger event, with only minor disturbances potentially present. It is relatively compact and appears to be a galaxy of intermediate mass.
