The galaxy presents as a relatively smooth, elliptical structure. Its light profile appears concentrated towards the center, with a gradual decrease in surface brightness extending outwards. The galaxy exhibits a yellowish-white hue, which is suggestive of an older stellar population. There is little indication of significant spiral arm structure or dust lanes within the galaxy. Based on its shape, it is highly likely that the galaxy is an elliptical galaxy. There does not appear to be any evidence of an ongoing major merger event, however a slight asymmetry could potentially be interpreted as evidence of a minor disturbance or past interaction. The central bulge is the brightest region of the galaxy.
