The galaxy presents a predominantly smooth morphology with a high degree of central concentration. It exhibits an overall elliptical shape, appearing somewhat flattened but not displaying a distinct disk structure. The central region is noticeably brighter and exhibits a reddish hue, possibly indicating an older stellar population or significant dust obscuration. Fainter, greenish-blue extensions surround the core, suggesting the presence of some younger stars or active star formation. These outer regions appear less structured and more diffuse. There is no visual evidence of major mergers or significant tidal disturbances. The color gradient, from a redder core to bluer outer regions, may indicate radial variations in stellar population ages or dust content.
