The galaxy presents as a relatively smooth, centrally concentrated structure. Its overall shape appears mostly round, exhibiting only a slight deviation from perfect circularity. There are no discernible spiral arms or bar-like features readily apparent. The light distribution suggests a centrally dominant bulge with a gradual decrease in luminosity towards the outer regions. The galaxy appears to be relatively isolated, with no obvious signs of a major ongoing merger or tidal disturbances. Color gradients indicate a likely transition in stellar populations and/or dust content from the core to the periphery. The core exhibits a yellow-ish color compared to the outer edges, which seem to be slightly bluer.