The galaxy exhibits a distinct spiral morphology. Two prominent spiral arms emanate from a central bulge. These arms are not tightly wound; rather they display a medium to loose winding pattern. The bulge appears moderate in size relative to the overall galaxy. There appears to be a weak bar feature within the central region. The disk of the galaxy appears relatively face-on with no edge-on features. Overall the galaxy shows minor disturbances perhaps indicating recent minor interactions. The galaxy exhibits colors indicating intermediate star formation rates. The color distribution suggests younger stellar populations are present within the spiral arms, while the central bulge may contain a higher proportion of older, redder stars. There may be a slight blueish tinge on one side, again indicating star formation in that region. 
