The galaxy presents as a relatively smooth, elliptical form. Its central region exhibits a bright, concentrated luminosity, gradually fading outwards into a diffuse halo. The overall color profile suggests a population of older stars, with a noticeable lack of strong blue star-forming regions. There appears to be a slight elongation, indicating a flattened spheroidal shape rather than a perfect sphere. Evidence of spiral arm structure or prominent dust lanes is absent, further supporting its classification as an elliptical galaxy. There may be very faint traces of tidal disturbance suggesting a past interaction or merger event.
