The galaxy appears to be a spiral type, presenting a face-on orientation. It exhibits two prominent spiral arms that wind moderately around a central bulge. There may be a weak bar-like structure within the bulge. The bulge itself seems to be moderate in size compared to the disk of the galaxy. The spiral arms appear somewhat flocculent, with regions of brighter star formation. The overall color suggests a mix of stellar populations. The galaxy doesn't obviously exhibit signs of major mergers, although some minor disturbances could be present. 
