The galaxy exhibits a generally smooth morphology, appearing largely elliptical in shape. The light distribution is concentrated towards the center, creating a bright, well-defined nucleus that suggests the presence of a supermassive black hole. Proceeding outward from the nucleus, the light gradually fades, defining a distinct galactic bulge. There is a discernible color gradient present. The central bulge is characterized by a yellowish-orange hue, suggestive of an older stellar population. The outer regions of the galaxy show a slight bluer tint. The overall lack of spiral arm structures or significant dust lanes further supports its classification as a galaxy in the elliptical to lenticular regime. There is a very slight asymmetry present, suggesting the possibility of a past interaction, but the dominant feature remains that of an undisturbed and well-formed galaxy.
