The galaxy presents as a centrally concentrated, relatively smooth object with a pronounced elliptical morphology. The color is generally yellowish-white, suggesting a stellar population dominated by older stars, although there appears to be a hint of bluer color in the center, which could imply some regions of ongoing, or recent, star formation. There are no visually discernible spiral arm structures or prominent dust lanes, and the light distribution appears fairly uniform across the galaxy's surface. The galaxy appears relatively isolated with no obvious signs of recent or ongoing major mergers or tidal disturbances. The light profile suggests a gradual decline in brightness from the core to the outer edges, typical of elliptical galaxies.
