The galaxy presents as a spiral type, exhibiting a disk-like structure. Prominent, loosely wound spiral arms are observable extending from the central bulge. The bulge itself appears moderately sized relative to the disk. Two spiral arms are clearly visible, appearing grand and well-defined. A bar may be present, bisecting the central region of the galaxy, although the presence of the bar is unclear. There is an overall blue tinge to the galaxy, especially within the arms, suggesting a high rate of ongoing star formation. There is no indication that this galaxy is currently undergoing any major merger events. The disk is being observed face-on.
