The galaxy presents as a spiral type, exhibiting well-defined spiral arm structures. The arms display a tightly wound morphology, and their azimuthal coverage is extensive throughout the galactic disk. Within these spiral arms, there are bright knots indicating regions of active star formation. The central bulge is relatively small and not particularly prominent in relation to the disk. A weak or no bar structure seems to be at the center. The galactic disk appears to be viewed at a close to face-on inclination. There is little to no sign of a major or minor merger event.
