The galaxy presents as a concentrated, elliptical-like structure. Its overall color profile suggests a composition of older stellar populations. The central bulge appears prominent and exhibits a smooth luminosity profile, indicating minimal dust obscuration. Faint diffuse light emanates from the galaxy, gradually fading into the background. There is no indication of spiral arms, bars, or tidal features. The galaxy's morphology suggests it is a relatively undisturbed system, having undergone little to no recent mergers. The relatively high round fraction suggests that this is an E0-E3 type elliptical galaxy.
