The galaxy presents as an elliptical or spheroidal system. It exhibits a centrally concentrated luminosity profile, with intensity decreasing smoothly outward from a bright, yellowish core. There is little evidence of spiral arm structure or significant dust lanes. The overall color is consistent with an older stellar population, lacking in significant ongoing star formation. It exhibits a generally smooth appearance and has little morphological disturbance suggesting a relatively relaxed dynamical state. The estimated size suggests it is a relatively large galaxy, and the smooth, round morphology is suggestive of an evolved system.
