The galaxy presents as a relatively smooth, elliptical structure. Its light is concentrated towards the center, displaying a bright, yellowish core. There is a slight color gradient visible extending outwards from this central region to a fainter, more diffuse halo. There is minimal evidence of spiral arm structures or dust lanes. The galaxy's overall shape is approximately round. There are no obvious signs of tidal tails, major distortions, or interacting companion galaxies, though subtle disturbances cannot be entirely ruled out based on this imagery alone. The stellar population appears dominated by older stars, consistent with a relatively low star formation rate.