The galaxy presents a complex morphology, with prominent spiral arms and a generally disk-like structure. The spiral arms appear to have varying degrees of winding, with a significant portion exhibiting tightly wound formations, although medium and loosely wound arms are also present. There's a suggestion of multiple spiral arms extending from the central region. The core region of the galaxy appears bright and relatively smooth, with an indication of a small bulge component. There is no strong indication of a bar-like structure traversing the central region, though a weak bar cannot be ruled out. Overall, the galaxy appears to be relatively undisturbed, with no strong visual signs of major mergers or significant tidal disturbances, although minor disturbances may be present.
