This appears to be a spiral galaxy exhibiting a moderate degree of spiral arm structure. The arms are somewhat flocculent, not tightly wound, with segments more prominent than others. There is a hint of a central bar feature. The bulge is relatively moderate in size, not a dominant feature, but distinctly present. Some indications of ongoing star formation in the disk. The overall appearance suggests the possibility of a minor interaction or disturbance in the galaxy's morphology. It is likely the galaxy is in a late stage of disk instability. The galaxy presents a relatively smooth appearance, but does have defined features, like it's bars. It is observed to not be edge on, and the arms can be observed to be a bit dispersed. 
