The galaxy presents as a roughly elliptical, spheroidal structure. The light profile is dominated by a smooth, centrally concentrated bulge, exhibiting a gradual decrease in surface brightness outward from the core. The core region appears a yellowish-white, suggesting a stellar population primarily composed of older, lower-mass stars. The outer regions of the galaxy display a slightly bluer hue compared to the core, which could indicate the presence of a younger stellar population. The galaxy does not display any strong spiral arm features, bars, or prominent dust lanes. There is no evidence of ongoing major mergers or tidal disturbances in this image; the overall morphology appears relatively undisturbed. The galaxy appears fairly compact with an appreciable size and consistent with an early-type galaxy.
