The galaxy exhibits a clear spiral structure, with arms extending outwards from a central bulge. The arms display moderate winding, neither tightly wound nor loosely defined. A substantial fraction of light emanates from these spiral arms. The galaxy is observed face-on, with a low inclination relative to our line of sight. There's evidence of a bar-like structure traversing the central region. The bulge appears relatively small compared to the overall size of the disk, but is not negligible. The presence of HII regions and other star-forming activity is suggested by the irregular patches of light. Overall, the galaxy appears to be in a relatively undisturbed state, with no immediately obvious signs of a major merger event. However, minor disturbances may be present in the outer regions. The spiral arms appear to have 2-3 main arms that are well-defined, though other arms appear to exist.
