The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, concentrated morphology. It appears largely spheroidal with a slight elongation along one axis, suggesting a possible disk component viewed at an oblique angle. The light profile is centrally concentrated with a gradual decrease in intensity outwards.

Color gradients are evident, with the core displaying a yellowish-orange hue, indicative of an older stellar population likely dominated by red giant stars. The outer regions appear slightly bluer, hinting at the presence of younger, hotter stars, although star formation appears generally suppressed. No prominent dust lanes or spiral arm structures are discernible. The galaxy does not appear to be undergoing any major mergers or tidal disturbances, presenting a relatively undisturbed, relaxed structure. Overall, it appears to be a relatively massive system with a significant bulge component.
