The galaxy presents a primarily smooth, elliptical morphology. A bright, concentrated nucleus dominates the galaxy's structure, surrounded by a more diffuse halo. The halo appears to fade gradually without distinct spiral arms or prominent features. The object exhibits a moderately flattened shape, neither perfectly spherical nor highly elongated, indicating an oblate spheroidal form. The color profile suggests a population of older stars, with a yellowish-red hue dominating the central bulge, which likely means star formation is quite low. No signs of major mergers or significant tidal disturbances are visually apparent.
