The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a nearly circular morphology. There is little evidence of distinct spiral arms or a prominent disk structure. The light distribution is dominated by a centrally located bulge, with a gradual decrease in surface brightness as one moves outward from the center. The galaxy possesses a cyan hue. There may be some minor indications of disturbance in the outer regions, but overall the structure appears largely undisturbed. The core seems to be very dense, and very energetic. 
