This galaxy presents as a smooth, elliptical form. It exhibits a high degree of central concentration with a bright, golden core. Moving outwards, the galaxy fades gradually into a diffuse halo. There is a slight elongation, suggesting a deviation from perfect sphericity, appearing more cigar-shaped than completely round. No prominent spiral arms or well-defined disk structures are discernible. The overall color profile suggests a relatively older stellar population, with a lack of intense blue regions indicative of recent star formation. There is no apparent evidence of ongoing mergers or major tidal disturbances affecting the galaxy's morphology.
