The galaxy presents as a somewhat elliptical structure with a concentrated central bulge. The core exhibits a yellowish-orange hue, suggesting a population of older stars. A bluer, diffuse disk surrounds the central bulge, indicating the presence of a younger stellar population and possible ongoing star formation. The disk is not perfectly smooth but shows hints of subtle features or disturbances, possibly indicative of minor gravitational interactions. Overall, the galaxy appears relatively undisturbed with a dominant smooth component.
