The galaxy presents a prominent disk structure. There appears to be a bright central bulge that is not overwhelmingly dominant, but certainly substantial. Spiral arms are present, although their morphology is somewhat difficult to discern due to the resolution; the arms appear rather tightly wound toward the center of the galaxy. The overall impression is of a galaxy exhibiting relatively ordered spiral structure. There are no obvious signs of major merger activity. Overall, the light distribution suggests a relatively face-on spiral galaxy, with the presence of a stellar population that is actively forming stars.

