The galaxy presents as a relatively smooth and somewhat elliptical structure. The central region exhibits a concentration of light with a yellowish-orange hue, suggesting a population of older stars. The outer regions appear more diffuse and less structured, with a slight decrease in color temperature. There is no discernible spiral arm structure visible, and the overall morphology appears relatively undisturbed. There is a slight indication of asymmetry to the isophotes. I observe little in the way of dust lanes or prominent star-forming regions.
