The galaxy exhibits a prominent spiral structure. The spiral arms appear loosely wound and well-defined, extending outwards from a central bulge. The bulge is of moderate size in relation to the overall galactic disc.  Two distinct spiral arms appear to dominate the structure. There is no strong evidence of a bar feature transecting the bulge.

There are signs of ongoing star formation within the spiral arms as indicated by bluer regions. The colour distribution of the galaxy is generally bluer in the disc relative to the bulge, as expected with ongoing star formation in the arms. There is no significant interaction or sign of a merger event and the galaxy does not appear to be a smooth elliptical.
