The galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The overall color appears to be a slightly bluish-white, with a hint of redder tones towards the galactic center. No distinct spiral arms are readily visible. The outer regions of the galaxy appear more diffuse and less structured than the central area, fading gradually into the background sky. The general form suggests a possible classification as an early-type spiral or a lenticular galaxy, possibly undergoing a relatively low rate of star formation. There is a slight asymmetry visible suggesting there might have been a past interaction or merger, or there might be some internal disturbance.
