The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that fades outward into a more diffuse halo. The core region displays a yellowish-white hue, suggestive of an older stellar population dominating the luminosity in that region. As the light extends away from the center, the galaxy's outer regions exhibit a faint bluish tint, possibly indicating the presence of a younger stellar population, though such regions are minimal. The overall roundness and lack of distinct spiral arms support classification as an elliptical galaxy, with no obvious signs of ongoing major mergers or significant tidal disturbances. There is no significant structure beyond this description that can be inferred.
