This galaxy presents as a roughly edge-on spiral, exhibiting a distinct disk shape. The central bulge appears to be prominent and exhibits a spheroidal morphology. The disk shows some indication of possible warping. The integrated color suggests a population of older stars, particularly in the bulge. Evidence suggests this galaxy is undergoing a low level of star formation. There appears to be a companion dwarf galaxy in the foreground creating possible tidal disturbances of the disk.
