The galaxy presents as a face-on spiral, with a well-defined disk structure. The spiral arms appear prominent and tightly wound, although it is difficult to discern their precise number due to some overlap. A significant portion of the arms seem to originate from the central region and extend outwards in a fairly symmetric manner. A bar structure is suggested, although not especially pronounced; if present, it seems rather weak. A bulge is present, seemingly of small to moderate size relative to the overall disk. There are no obvious signs of major merging activity, although some minor disturbances or asymmetries in the disk's morphology could be suggestive of past or ongoing interactions. The galaxy exhibits a blue hue. The color suggests ongoing star formation within the disk and spiral arms.
