The galaxy presents as a relatively smooth, elliptical structure. It appears to be nearly face-on, exhibiting a moderate degree of ellipticity. The light distribution suggests a centrally concentrated bulge, characteristic of early-type galaxies. The color gradient indicates a population of older stars, with a yellowish-red hue dominating the core, and potentially some bluer regions in the outer areas. There are no prominent spiral arms or dust lanes visible. The overall morphology suggests a well-evolved system that has likely undergone significant internal evolution. There are no obvious signs of recent major mergers or tidal disturbances.
