The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse light profile. There is a distinct lack of discernible spiral arms or significant dust lanes. The core exhibits a yellowish-white hue, indicative of an older stellar population, while the outer regions appear slightly bluer. There are no obvious signs of major mergers or tidal distortions, though there may be a very subtle asymmetry suggesting a minor interaction in its past. The overall shape appears mostly rounded, with a slight elongation. 
