The galaxy presents as a relatively smooth, elliptical morphology with an apparent color index suggesting a population of older stars. It shows an elongated shape, with a length approximately twice its width. The light distribution is concentrated towards the center, fading gradually towards the edges. There is no visible evidence of spiral arms or significant dust lanes. The galaxy does not appear to be strongly interacting or undergoing a major merger, although there are subtle irregularities in its outer regions that may indicate a minor disturbance or past interaction. Overall, it is a relatively quiescent galaxy with a smooth, featureless structure and a likely low star formation rate.
