The galaxy presents as a single, fairly symmetrical object with a smooth, concentrated appearance, suggesting an elliptical morphology. The light profile is centrally concentrated, with a core that is significantly brighter and more yellow than its outer regions. The outer regions are a deeper red, indicating the presence of an older stellar population. There is little evidence of spiral arms or significant dust lanes. The galaxy is relatively undisturbed with no signs of tidal tails or other major merger signatures. The galaxy appears to be relatively round in shape. Overall, the galaxy appears to be a well-formed elliptical with a dominant, older stellar population and very little ongoing star formation.
