The galaxy presents as a singular, relatively smooth object with minimal discernible substructure. Its overall shape is largely circular, exhibiting high degree of sphericity. The light distribution across the galaxy is centrally concentrated, with a gradual decrease in intensity radiating outwards, lacking any distinct spiral arms or bar features. There is a slight colour variation across the galaxy, more blue closer to the core and slightly redder toward the outer edges. There is a small asymmetry in the light distribution on one side, indicative of a potential minor gravitational interaction.
