The galaxy presents a largely smooth, elliptical morphology. It appears centrally condensed, with a gradual decrease in luminosity extending outwards. The color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue, although some green can be seen. There is no discernible disk structure or spiral arm pattern, implying a relatively quiescent state. The galaxy seems undisturbed, lacking any significant signs of tidal interactions or ongoing merger activity. The shape appears mostly round. Overall, the galaxy seems to be a relatively evolved, early-type system.
