The galaxy presents a primarily smooth and elliptical morphology. Its core region exhibits a bright, concentrated luminosity, transitioning to a dimmer halo extending outwards. The overall color is predominantly redder, suggesting an older stellar population. The visible structure lacks defined spiral arms or prominent dust lanes. It seems to be an early-type galaxy with no apparent signs of major mergers, only a slight possible minor disturbance. The galaxy appears generally unperturbed.
