The galaxy presents a largely smooth morphology, indicative of an elliptical galaxy. It exhibits a predominantly round shape with a slight degree of ellipticity. The galaxy appears centrally concentrated with a gradual decrease in luminosity towards its outer regions. There is no visible evidence of spiral arm structures or prominent dust lanes. No signs of ongoing major mergers are apparent, although there might be minor disturbances in the morphology, which could be the result of a past interaction with a smaller galaxy or a minor merger event. The overall color is reddish, which suggests an older stellar population with relatively low levels of current star formation. The galaxy is a considerable distance away.
