The galaxy exhibits a clear spiral structure with two prominent arms emanating from a bright, moderately sized central bulge. The spiral arms appear somewhat flocculent, with medium winding and contain regions of active star formation, indicated by bluish hues. The galaxy does not appear to be viewed edge-on. There is an indication of a possible bar structure across the center of the galaxy. There are some morphological disturbances and the overall appearance is somewhat irregular which suggests possible tidal interactions or ongoing minor merger events. The galaxy color suggests that it has intermediate mass and star formation rate.