The galaxy presents a distinct spiral morphology, displaying prominent, well-defined spiral arms. The winding of these arms appears to be of medium tightness. A significant fraction of the light emanates from these spiral structures.

The central bulge is of moderate size, exhibiting a yellowish hue which may indicate an older stellar population. The galaxy does not appear to be edge-on. There is no obvious indication of a strong bar structure traversing the nucleus. Similarly, there is no evidence to suggest this galaxy is undergoing a major merger, though minor disturbances cannot be ruled out based on visual inspection alone.
