The galaxy presents a multi-component structure, exhibiting a mix of smooth and featured characteristics.  A dominant disk is visible, although it is not observed edge-on. Within the disk, spiral arm structures are readily apparent.  A bulge is present, estimated to be moderate in size.  Evidence suggests a possible bar feature extends across the central region of the galaxy. There are indications of a possible interaction or disturbance within the galaxy, suggesting a possible merging event. The galaxy displays a bluer color in the central portion of the disk, then tends toward redder hues in the outer reaches.

