The galaxy presents as a relatively smooth, round object. It appears to have a concentrated central bulge which diffuses outwards with no clear spiral arm structure. The galaxy exhibits a yellowish-red color gradient, suggesting a population of older stars and a low ongoing star formation rate. The central region is brighter and more yellow, potentially indicating a higher concentration of older, evolved stars, while the outer regions appear slightly redder and more diffuse. There are no apparent signs of major mergers or tidal disturbances in this image, which could point toward a relatively isolated evolution. Faint disk-like components may be present but are not easily distinguished due to the smoothness.
