The galaxy appears to be a luminous, centrally concentrated object, likely an elliptical galaxy, exhibiting a smooth morphology. Its light is dominated by a yellow-white hue near the core, suggesting an older stellar population. The outer regions fade in intensity and appear more bluish, possibly indicating some younger stars. The galaxy shows a generally rounded shape with no obvious signs of a disk structure or spiral arms. No major disturbances or prominent tidal features are visible, which indicates that this galaxy is likely not undergoing a major merger event. The radial light profile suggests a gradual decrease in brightness from the core outwards. Overall, it presents as a mature, relatively undisturbed system.
