The galaxy presents as a largely smooth, elliptical structure with a concentrated, bright central bulge. The light profile transitions gradually from the core to the outer regions. There is a subtle color gradient, with a yellowish-white hue dominating the central region and shifting towards a slightly bluer tone in the surrounding areas.  The galaxy exhibits a high degree of rotational symmetry, indicating it is not undergoing any major mergers or strong tidal interactions. There are no visually prominent spiral arms, bars, or dust lanes visible. Faint, diffuse extensions of the galaxy's halo seem to spread out from the main body but they are very small and faint. The galaxy shows a small amount of star formation.