The galaxy presents as a single, concentrated luminous object. It appears to be a relatively smooth, elliptical galaxy lacking prominent spiral arms or a distinct disk structure. The galaxy exhibits a centrally concentrated light profile, with a gradual decrease in luminosity moving outwards from the core. Its overall shape is generally round. There are no indications of ongoing major mergers or tidal disturbances. The color is yellowish-orange, which suggests a population of older stars, and possibly a low rate of star formation. The light is dominated by evolved stellar populations.
