The galaxy appears to be a spiral galaxy viewed edge-on. There is a prominent dust lane bisecting the galaxy, obscuring the central bulge. The bulge seems to be more rounded than boxy. The disk appears relatively smooth and shows minimal signs of disturbances, such as tidal tails or asymmetries, suggesting it has not recently undergone a major merger. The galaxy shows a slight color gradient, trending from blue to yellow with the red end fainter, which hints at areas of more intense star formation. The extent of the galactic disk is moderate. Based on the observed morphology, the galaxy is likely to be relatively quiescent with a low star formation rate.
