The galaxy presents as a relatively smooth, disk-like structure. There appears to be a bulge, possibly a bar or a very elongated bulge. The color of the galaxy appears primarily yellowish or green, particularly in the central region, suggesting a population of older stars. However, there may be some indication of star formation or hotter gas evident in the reddish regions. The overall roundness of the galaxy appears to be more in between disk-like and spheroid. There are signs of minor tidal disturbance, but not major merging is occuring.