The galaxy presents a generally smooth, elliptical morphology. It displays a centrally concentrated luminosity profile with a relatively high degree of circular symmetry. There is minimal visual evidence of spiral arm structures or prominent dust lanes. There is a very subtle hint of an extension or tidal feature extending from the main body of the galaxy suggesting that the galaxy may have undergone a past interaction with another galaxy. There is no indication of recent or current star formation. The galaxy appears relatively massive.
