The galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is a slight elongation, deviating from a perfectly circular shape. The galaxy exhibits a color gradient, with a redder core transitioning to a bluer halo. The lack of distinct spiral arms or prominent dust lanes indicates a relatively quiescent galaxy, possibly an early-type system. There are no obvious signs of major mergers or significant tidal disturbances.
