The galaxy presents as a relatively smooth, elliptical-like structure. The light profile appears centrally concentrated, exhibiting a gradual decrease in intensity outwards. The overall color is slightly redder, suggesting an older stellar population. There is no apparent disk structure or spiral arm features visible within the galaxy's morphology. Faint hints of asymmetrical extensions or tidal features are not definitively ruled out. The galaxy appears relatively undisturbed and isolated based on current resolution. 
