The galaxy presents as a moderately luminous, well-defined elliptical system. It appears relatively smooth in texture with no immediately obvious dust lanes or spiral arm structures. Its light profile suggests a concentrated nucleus with a gradual decrease in surface brightness towards its outer edges. The overall color of the galaxy seems slightly bluer than that of a typical elliptical, possibly indicating some degree of recent or ongoing star formation, although it appears to be at a low rate. The morphology is generally undisturbed, showing no significant signs of tidal interactions or recent merger events. The galaxy is not perfectly circular, displaying a slight ellipticity.
