The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. It exhibits a somewhat yellowish hue in the central region, suggesting an older stellar population. The outer regions appear fainter and more diffuse, transitioning into a surrounding halo. There is only a hint of a disk-like structure, with little indication of spiral arms or significant dust lanes. There appear to be some minor disturbances in the outer regions, but overall the galaxy appears to be relatively isolated, without any obvious signs of a major ongoing merger. The shape tends towards being round rather than elongated.
