The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a central bulge that dominates its overall structure, surrounded by a more diffuse halo. There is a slight elongation to the galactic disk, indicating it is not perfectly spherical. Color gradients suggest a higher concentration of older stellar populations towards the center, with slightly bluer hues in the outer regions, hinting at ongoing, though subdued, star formation. The overall light distribution is concentrated, with a rapid falloff in brightness as you move away from the core. No distinct features such as spiral arms or dust lanes are visible.
