The galaxy presents as a nearly face-on elliptical morphology. It exhibits a smooth, diffuse light distribution, with a bright, concentrated core region. There is a very faint flattening in the outer regions, suggesting a slight ellipticity. The galaxy displays a distinct color gradient, transitioning from a bluer hue near the core to a redder tone in the outer regions. This suggests the presence of younger, hotter stars concentrated in the central regions, while the outer regions are populated by older, cooler stars. There are no obvious signs of spiral arms or significant dust lanes. The overall appearance indicates a relatively evolved system.
