The galaxy appears as a relatively smooth, elliptical object with a prominent bulge. The central region exhibits a reddish hue, potentially indicating an older stellar population. The outer regions display a greenish tinge, which could be attributed to the presence of younger stars or ongoing star formation activity, albeit at a low rate. The galaxy does not show significant signs of spiral arms or a well-defined disk structure. There is no obvious indication of a major merger event, although minor disturbances are possible. The overall morphology suggests a galaxy that is relatively evolved and possibly undergoing a transition in its star formation history. Its apparent roundness implies that it is closer to being face-on.
