The galaxy appears as a centrally concentrated, largely featureless spheroid. The light is dominated by a smooth, bright core that gradually fades into a more diffuse halo. There is a slight elongation observable, but it is generally round. There is little evidence of spiral arms or dust lanes. The color profile suggests a population of older stars with a slight bluer tint in the central region compared to the edges, possibly indicating a low level of ongoing star formation. Overall, the galaxy presents as a relatively undisturbed system with no obvious signs of recent major mergers or interactions.
