This galaxy appears to be a relatively smooth, elliptical type. It exhibits a central bulge that is brighter and more concentrated, surrounded by a more diffuse halo. The galaxy's overall shape is somewhat elongated, rather than perfectly spherical. There is a slight hint of bluer light on the periphery of the disk, suggesting some ongoing star formation, although it is not prominent. There are no obvious signs of strong tidal interactions or major disturbances, though some minor irregularities are present, suggesting the possibility of a past or ongoing minor merger event. The overall color gradient indicates a population of older stars, especially within the core. The galaxy is likely a moderate mass system.
