The galaxy presents as a somewhat elliptical, relatively smooth system. Its central region exhibits a bright, concentrated yellow-white luminosity, indicating a population of older stars. The outer regions show a gradual decrease in surface brightness, with hints of bluer tones, which might suggest some recent or ongoing star formation, albeit at a low rate. There is no obvious spiral structure or pronounced dust lanes visible, which might classify it as a lenticular or early-type spiral galaxy seen from a relatively face-on orientation. Overall, the galaxy appears well-defined with a compact structure.
