The galaxy presents an overall elliptical morphology, although it is not perfectly spherical. The light distribution is smoother than that of a typical spiral galaxy, with a centrally concentrated bulge. The core of the galaxy exhibits a yellowish-white color, indicating a population of older stars. Moving outward from the core, there's a transition to a bluer hue in the outer regions, suggesting the presence of younger stars or ongoing star formation, albeit at a moderate rate. Faint and slightly disturbed arms seem to surround the galaxy. No major mergers or intense tidal interactions are visually apparent. The galaxy appears relatively isolated.
