The galaxy presents as a centrally concentrated, relatively smooth object with a dominant spheroidal morphology. Its overall color is slightly reddish-yellow, indicating a significant population of older stars and potentially substantial dust obscuration. There is no clear evidence of spiral arms or a distinct disk component. The galaxy appears largely undisturbed, lacking prominent tidal features or signs of ongoing mergers. Its shape is close to circular, with only a slight deviation towards being in-between circular and elongated. The light profile appears to gradually decrease in intensity from the core to the outer regions, suggesting a relaxed stellar distribution within the galaxy.
