The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse appearance. A distinct, bright core is visible, surrounded by a more extended, fainter halo. The light distribution is consistent with an early-type galaxy, possibly an elliptical or lenticular type. There are hints of subtle color gradients within the galaxy, with the core appearing slightly redder than the outer regions which appear more blue. There does not appear to be any dust lanes or spiral arm structures. The galaxy appears relatively undisturbed, without any obvious signs of major mergers or tidal interactions. Overall, the galaxy exhibits a relatively high degree of symmetry and regularity in its morphology.
