The galaxy presents as a somewhat smooth, centrally concentrated object. The light distribution appears relatively even, with no prominent spiral arms or distinct features immediately apparent. There is a slight elongation, indicating it is not perfectly circular, trending towards a more elliptical shape. The core is bright and intense, transitioning into a slightly diffuse halo, with the outer regions fading gradually into the background sky. There is a hint of a disturbance in the overall symmetry; the edges are not entirely smooth, potentially indicative of minor tidal interactions or past merger events, but it is most likely a result of a smooth spheroid. The color seems to be yellow indicating an older, redder population of stars dominates. No dust lanes are visible within the disk. The overall structure suggests an elliptical galaxy, potentially undergoing minor interactions or possessing subtle internal disturbances.