The galaxy presents an elongated, elliptical morphology. Its light distribution appears concentrated towards the center, exhibiting a smooth, centrally-bright profile. Some apparent disturbances present that may be mergers. The primary body displays a color gradient, shifting from bluer hues near its upper section, to redder tones toward the center, potentially indicating differing stellar populations. There appear to be some disturbances or possible interactions with another object, or a merger in progress. Overall the galaxy's morphology and color distribution suggest an evolving system undergoing dynamic processes.
