The galaxy presents as a single, relatively compact object with a smooth, well-defined structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The overall shape is close to circular. Subtle color variations are discernible. The central region exhibits a slight yellowish-white hue, suggesting an older stellar population. Fainter, bluer tones may be present in the galaxy's outer regions. There is no clear evidence of spiral arms, bars, or other distinct features, nor any evidence of strong tidal distortions or ongoing merger activity. 
