The galaxy presents as a moderately luminous, relatively compact object with a smooth, elliptical morphology. A dominant, centrally concentrated bulge of older stars appears as a diffuse yellowish glow. There is minimal evidence of spiral arm structure or dust lanes within the visible wavelengths. The galaxy's overall color suggests a population of primarily evolved stars, with potentially low levels of ongoing star formation. It appears to be a relatively undisturbed system, showing no major signs of tidal interactions or recent mergers. The shape is mostly rounded. There is a faint, diffuse halo surrounding the galaxy, but it does not extend far from the central region.