The galaxy appears as a somewhat flattened spheroid. It exhibits a smooth, centrally concentrated light profile with a bright nucleus. There is a noticeable color gradient, shifting from a bluer hue in the outer regions to a redder hue towards the center, suggesting a differential distribution of stellar populations. The galaxy shows a slight elongation, indicating it is not perfectly circular. Overall, it appears relatively undisturbed, with no obvious signs of recent major merger activity.
