The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a near-circular morphology, with a gradual decrease in luminosity from the core outwards. A slight color gradient is observed, with the central region appearing somewhat redder than the surrounding halo. There is very little evidence of spiral arm structure or dust lanes. Faint, diffuse features potentially indicate some minor gravitational interaction, but it is generally isolated and undisturbed. The overall appearance suggests it is a mature galaxy with a significant population of older stars.
