The galaxy exhibits a clear spiral structure. Two distinct spiral arms are visible emanating from a central bulge. The winding of these spiral arms is moderately tight. The central bulge appears prominent, but not dominant, in size relative to the disk. The galaxy is not viewed edge-on, instead providing a near-perpendicular view of the disk. There is no apparent bar structure. No major mergers or significant disturbances are present in the galaxy's morphology.
