The galaxy exhibits a clear disk-like structure, viewed at a significant inclination. The central bulge is prominent and appears relatively smooth. The disk shows evidence of spiral arms. There is a subtle green hue, indicating a degree of on-going star formation. A slight asymmetry is present in the outer regions of the disk, possibly suggesting a past interaction or minor disturbance. The overall morphology is somewhere between a smooth elliptical galaxy and a spiral galaxy. The outer regions of the galaxy fade gradually, indicating a diffuse halo. The color gradients from the center outwards suggest a changing stellar population and/or dust distribution across the galaxy.