The galaxy exhibits a clear spiral structure. Predominantly, two distinct spiral arms appear to originate close to the central bulge, and wrap around the galaxy. The spiral arms have a moderately tight winding. The central bulge appears relatively small. The disk is not perfectly face-on, presenting a slight inclination. A weak bar structure may be present traversing the central region of the galaxy. No significant mergers or major disturbances are evident in the galactic morphology, though minor disturbances may be present. The galaxy has a prominent disk component, with ongoing star formation.