The galaxy presents as a largely featureless spheroid, indicative of an elliptical morphology or a lenticular galaxy seen face-on. There is a high degree of central concentration, with a bright nucleus that fades outward into a diffuse halo. The overall color is generally consistent with an older stellar population, though subtle color variations suggest the presence of some younger stars or dust. A slight extension in one direction might hint at tidal interactions or a faint disk component, but the limited resolution makes this difficult to confirm. Based on the smooth appearance, the galaxy appears to be relatively undisturbed.
