The galaxy appears as a smooth, centrally concentrated object with a somewhat elliptical morphology. It presents a yellowish-orange hue, suggesting a population dominated by older stars. There is minimal evidence of spiral arms or active star formation regions within the visible light spectrum. The overall structure seems undisturbed, although there are some hints of a minor disruption in the overall smoothness of the galaxy. It's relatively compact in size and it does not show an obvious disk structure. The light distribution decreases gradually from the center outwards.
