The galaxy exhibits a relatively smooth morphology with a central, bright bulge that appears roughly circular. Surrounding the bulge is a flattened disk structure. The disk is not uniformly bright; there appears to be some substructure or spiral arm fragments, although they are not well-defined. The color distribution in the galaxy is not uniform. The central bulge appears more yellow/white, indicative of older stellar populations. The disk shows bluer regions interspersed with redder areas, suggesting ongoing star formation alongside older stars. Diffuse light extends from the main body of the galaxy, particularly along the plane of the disk, possibly representing a halo or tidal debris. Overall, the galaxy shows only slight visual signs of disturbance and merging and appears to be a relatively undisturbed disk galaxy.
