The galaxy exhibits a disk-like structure, viewed at an angle somewhere between face-on and moderately inclined. A central bulge is present, appearing moderate in size relative to the overall disk. Evidence of spiral arm structure is discernible; however, they are not sharply defined. These arms show signs of active star formation. There also seems to be evidence of a small bar running through the central bulge. It looks like it is merging with or there is minor disturbance with another galaxy. Overall, the galaxy's color is slightly blue, suggesting a moderately active star formation rate.
