The galaxy presents a somewhat elliptical morphology. The central region exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a dense stellar population. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or significant dust lanes. There is a faint, elongated extension visible on one side of the galaxy, which could be a tidal tail or a minor disturbance caused by a past interaction or merger event. The overall color of the galaxy appears to be slightly on the bluer side.
