The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The light is concentrated towards the galactic center. The core exhibits a notably brighter, more yellow-white hue, possibly indicating an older stellar population. The outer regions transition to a fainter, slightly bluer color, which may imply a somewhat younger stellar population. The shape is not perfectly spherical. There are no readily apparent spiral arms or dust lanes, supporting a classification as an elliptical galaxy. No merging or major tidal disturbance can be discerned. The galaxy is viewed at a non-extreme inclination, with a slightly elongated profile.