The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellow-orange hue, suggesting a population of older stars. The galaxy displays a moderate ellipticity; it is elongated with an approximate ratio of 2:1, appearing somewhere between round and cigar-shaped. There are no obvious signs of spiral arms or significant dust lanes. The outer regions of the galaxy are fainter and blurrier, indicating a gradual decrease in stellar density with increasing distance from the center. There is no significant distortion or tidal features indicating recent major merger activity, though some minor disturbances can not be ruled out. The overall morphology suggests a galaxy that has largely completed the process of star formation and is now dominated by older stellar populations.
