The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. There is a distinct central bulge which appears yellowish-orange in color, suggesting a population of older stars. Surrounding the bulge is a more diffuse and slightly bluer halo, indicative of a younger stellar population and possibly ongoing, low-level star formation. The overall shape is elliptical, appearing nearly circular with only a slight elongation. No spiral arms or dust lanes are clearly discernible. There is no significant evidence of tidal interactions or recent mergers.
