The galaxy presents as a spiral type, although the disk is not perfectly face-on. Distinct spiral arms are visible, exhibiting a primarily two-armed structure. The arms display a moderate winding, neither tightly wound nor fully open. The central bulge appears relatively small, exhibiting a moderate size compared to the overall disk. There is no presence of a prominent bar feature bisecting the galaxy's central region, although a faint one may exist. The overall structure appears largely undisturbed, with no major signs of ongoing merger activity, although there are disturbances present in the galaxy. The galaxy displays a blueish hue overall, indicative of ongoing star formation within the spiral arms.
