The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a near-spherical morphology, with a slight elongation discernible along a north-south axis. The color profile is dominated by a bluish-white hue in the central region, suggestive of a population of younger, hotter stars. This central color gradually transitions to a slightly redder, more diffuse halo. There is no obvious spiral structure or prominent dust lanes visible within the galaxy, supporting its classification as an early-type system. No indication of any major mergers or significant tidal disturbances are seen.
