The galaxy presents as a smooth, centrally concentrated object. It exhibits a near-circular morphology, with no obvious signs of a disk structure or spiral arms. The central region is very bright and luminous, exhibiting a yellow-white hue, suggesting a population of older stars. Moving outward from the core, the galaxy displays a gradual decrease in surface brightness, fading into the background sky. There are some faint indications of a slightly bluer color in the outer regions, potentially indicating pockets of younger stars. There are no visible signs of major mergers or tidal disturbances.
