The galaxy presents as a centrally concentrated object with a relatively smooth, diffuse morphology. Its color profile suggests the presence of a slightly older stellar population, with a subtle color gradient implying redder hues towards the central region and bluer tones extending outwards. It is not perfectly spherical, appearing somewhat elliptical in shape. There is no readily apparent spiral structure, bar, or strong tidal features to indicate recent major merger activity, though a slight asymmetry hints at possible minor disturbances. 
