The galaxy presents as a single, dominant spheroid. The light profile appears smooth and centrally concentrated, with a gradual falloff in intensity from the core to the outer regions. The galaxy exhibits a slightly elliptical shape, though it leans towards round. There is subtle asymmetry, potentially indicating a minor gravitational disturbance in its recent past. Its color suggests a population of older stars, with a possible mild contribution from ongoing star formation. There are no obvious tidal features or signs of a major merger event. The overall appearance is consistent with a relatively massive galaxy undergoing moderate star formation.
