The galaxy presents as a spiral, viewed at an oblique angle, but not perfectly edge-on. The disk structure is evident, exhibiting discernible spiral arms that appear somewhat flocculent.  The arms are punctuated by regions of enhanced luminosity, suggestive of active star formation.  The central bulge appears relatively small and subdued, with the majority of the light emanating from the disk. There is some evidence of a possible interaction or merging event, exhibiting some degree of morphological disturbance. 
