The galaxy presents as a spiral type, with a disk inclined somewhat edge-on to our line of sight. There is evidence of some asymmetry in the disk structure. The central bulge appears prominent and has a yellowish color, suggesting an older stellar population. The arms exhibit a bluer hue, indicative of ongoing star formation. Patches of brighter blue regions are scattered throughout the disk. The light appears to be disturbed in some areas, which could indicate minor interactions or internal disturbances.
