The galaxy presents a largely smooth, elliptical morphology. It has a compact appearance, suggesting a relatively small size. The light distribution is highly concentrated towards the center, indicating a prominent galactic nucleus or bulge. No distinct spiral arms or disk-like features are discernible; instead, the light fades gradually from the core outwards, forming a diffuse halo. The galaxy appears nearly circular in shape, showing only a slight deviation from perfect roundness. There is no clear evidence of significant tidal distortions, ongoing mergers, or major disturbances in its morphology, suggesting it is likely a relatively undisturbed system. The color is most notable in the G and R bands.