The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that transitions smoothly outward. Color gradients suggest the presence of an older stellar population, with a predominantly yellowish-orange hue dominating the central region. This could indicate a low ongoing star formation rate. The outer regions of the galaxy show a gradual fading and are tinged with blue, potentially due to a small amount of younger stars or a slight contribution from dust scattering. The overall shape is mostly regular, showing no signs of strong tidal disturbances or major mergers. Slight asymmetry may exist, but is not severe.
