The galaxy presents an elliptical morphology, appearing relatively smooth with a central bulge that is bright and concentrated. The core region displays a yellowish-white hue, potentially indicating an older stellar population. A faint, extended halo surrounds the central region, exhibiting a greenish tint that could be attributed to ionized gas emission or a population of younger, hotter stars. There are hints of possible tidal disturbances or minor interactions. The disk appears relatively undisturbed, but there are some areas of asymmetry or slight warping that might be due to minor merger events or other gravitational disturbances. 
