The galaxy presents as a largely smooth, centrally concentrated object. It appears primarily elliptical in shape, with a high degree of radial symmetry. The core is bright, suggesting a concentrated stellar population and/or active galactic nucleus, appearing yellow-white in color, potentially indicative of older stars. Moving outward from the core, the galaxy displays a diffuse halo. The outer regions are more blue-shifted than the core, suggesting a younger stellar population, with the hint of a disk structure. No spiral arms or significant dust lanes are discernible. There is no obvious evidence of recent major mergers or significant tidal disturbances affecting the main structure of the galaxy.
