The galaxy presents as a centrally concentrated object with a generally smooth appearance. The core region exhibits a yellowish-white hue, suggesting an older stellar population. There is a more diffuse, bluish halo surrounding the central region, possibly indicative of ongoing or recent star formation. The object is largely spheroidal, exhibiting a high degree of circularity. There is no apparent evidence of major mergers or significant tidal disturbances. Faint wisps are seen, indicating minor disturbances.
