The galaxy presents a disk-like structure, observed at an oblique angle. Evident spiral arm features are present, though somewhat ill-defined, exhibiting a flocculent morphology.  A central bulge is discernable, appearing moderately sized and relatively bright.  There appears to be a significant interaction or merging event present as indicated by a distorted morphology in the galaxy disk. Some tidal features such as stellar streams or dust lanes are possibly visible.  The color suggests some areas of active star formation, and the overall galactic light is moderately bright.
