The galaxy presents as a disk galaxy, observed at a slight angle, but not quite edge-on. The galaxy's light suggests a moderately sized bulge. The disk component is evident and exhibits spiral arm structure. These arms appear somewhat flocculent. Color gradients within the galaxy suggest star formation. A bar structure is not obvious, although a slight elongation is noted. There is no clear indication of a major ongoing merger, though minor disturbances cannot be ruled out. The overall morphology suggests the galaxy is dominated by its disk, with a prominent but not overwhelming bulge.
