The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a bright, concentrated central bulge that fades gradually into the outer regions. The overall shape is somewhat rounded, showing a slight deviation from a perfect circular form. There is faint evidence of some minor irregularities or features within the diffuse outer halo, but nothing that would indicate a major interaction or ongoing merger event. Color gradients are present, with the central bulge appearing more yellow-white, suggesting an older stellar population, and the outskirts showing a slightly bluer hue.
