The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing mostly round in projection. The galaxy's core is compact and displays a reddish hue, indicating a potentially older stellar population or the presence of dust obscuration. Surrounding the core, a more diffuse, bluish halo is observed, suggesting the presence of a younger, hotter stellar population undergoing active star formation. There is no apparent spiral structure or distinct disk. The outer regions fade gradually into the background, and there's no visual evidence of strong tidal features or ongoing major mergers, though a slight asymmetry cannot be ruled out completely. The overall color gradient, from redder core to bluer outer regions, points to an inside-out formation scenario or differential dust extinction.
