The galaxy appears as a relatively smooth, centrally concentrated object with a nearly circular morphology. There is a subtle color gradient observable, with the central region exhibiting a slightly bluer hue compared to the outer regions, which appear redder. The overall light distribution indicates a system that is not dominated by spiral arms or strong bar features. The relative smoothness suggests a well-mixed stellar population, potentially indicative of an elliptical galaxy or a lenticular galaxy viewed face-on. The slight blueness of the central region suggests the presence of some ongoing, albeit low-level, star formation activity. There is no obvious evidence of major tidal disturbances or recent mergers in the immediate vicinity of the galaxy.
