The galaxy appears as a concentrated, smooth object with a primarily elliptical morphology. It exhibits a dominant central bulge characterized by a yellowish-orange hue, suggesting a population of older stars. The light is relatively uniform across the galaxy, and the shape appears very round. There may be some minor disturbance or a very faint merger event occurring but the light is too concentrated to be certain. Overall, the galaxy presents as a well-formed, relatively undisturbed system.
