The galaxy presents as a relatively smooth, elliptical-like structure, though not perfectly spherical. The central region displays a concentrated luminosity, suggesting the presence of a prominent galactic bulge. The color profile indicates an older stellar population, with a yellowish-white hue dominating the core. Fainter, bluer light is subtly visible in the outer regions of the galaxy, potentially indicative of some ongoing, though subdued, star formation. There is a slight irregularity in the shape of the galaxy, which may be due to a minor interaction. Overall the galaxy appears to be a relatively undisturbed system.
