The galaxy presents a generally smooth and centrally concentrated morphology, suggestive of an elliptical galaxy or a lenticular galaxy viewed face-on. The central region exhibits a bright, yellowish hue, potentially indicating an older stellar population. Proceeding outward from the center, the light gradually diminishes in intensity, forming a less defined, diffuse halo. A faint, bluish tint is observed in the outer regions, possibly indicating the presence of younger stars or ongoing star formation, though this is not pronounced. There's a very slight indication of a disk structure. Overall, the galaxy appears relatively undisturbed with no clear signs of ongoing mergers or major tidal interactions.
