The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its core presents a bright, yellowish-white hue, suggesting a population of older stars. The light gradually fades towards the outer edges, with a subtle transition from yellow to a slightly reddish tone, indicating possible differences in stellar populations or dust distribution. No distinct spiral arms or bar structures are discernible within the galaxy's disk. There are no signs of ongoing major mergers or significant tidal disruptions. A hint of possible minor disturbances might be present in the outer halo. Overall, the galaxy seems relatively undisturbed and well-defined.
