The galaxy exhibits a prominent disk structure with well-defined spiral arms. These arms are relatively tightly wound near the central bulge region, but become more loosely wound as they extend outwards. Two main spiral arms appear to be present.

A moderate-sized central bulge is visible, although it does not dominate the overall structure of the galaxy. A strong bar feature crosses the central region of the galaxy.

There appears to be some evidence of a minor disturbance.
