The galaxy presents a relatively smooth, elliptical morphology. Its shape is approximately round, exhibiting only a slight elongation. There is no evidence of a distinct disk or spiral arms. The central region appears brighter than the outer areas, suggesting a concentration of stars towards the galactic nucleus. The galaxy displays a color gradient, shifting from a somewhat bluer hue in the center to redder tones at its periphery. Based on the red color and smooth morphology, the galaxy is likely an evolved system. There are no obvious signs of ongoing major mergers, although some minor disturbances cannot be ruled out.
