The galaxy presents as a spiral, viewed at a moderate inclination angle relative to our line of sight. Two distinct spiral arms are visible. These arms appear tightly wound around the central bulge. The spiral arms are identifiable by their bluer coloration. The central bulge appears more yellow, suggesting an older stellar population in this region. There appears to be a bar feature across the center. The central bulge is moderately sized. The disk of the galaxy appears to be relatively undisturbed, with no obvious signs of a major merger event. There is a notable degree of dust obscuration visible. The spiral arms appear somewhat fragmented.