The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a moderately elliptical morphology, appearing somewhat flattened. The color profile suggests an aging stellar population. The galaxy lacks the distinct features of spiral arms or prominent dust lanes, indicating a more evolved or quiescent state. There are no obvious signs of recent or ongoing major mergers or tidal disturbances. The galaxy's core appears bright, with a gradual decrease in luminosity towards the outer regions.
