The galaxy presents as a relatively smooth, elliptical object with a high degree of central concentration. Its shape is somewhat elongated, tending toward a cigar-shaped morphology. The core region exhibits a bright, yellowish-white color, suggesting an older stellar population. The outer regions appear fainter and slightly redder, potentially indicating the presence of some dust or a population of cooler stars. There is no visual evidence of strong spiral arms or disk-like features. The overall appearance is largely undisturbed, with no obvious signs of ongoing major mergers or significant tidal disruptions, although subtle minor disturbances cannot be ruled out.
