The galaxy presents as a spiral galaxy with a significant disk component. Spiral arms are visible, displaying a moderate degree of winding. The central bulge appears moderate in size, contributing substantially to the galaxy's overall luminosity. There is a notable presence of a bar-like structure spanning across the central region of the galaxy. The disk appears face-on. The dust lanes can be seen within the disk. The overall color of the galaxy appears bluish, indicating recent star formation. There appears to be no significant signs of disruption indicative of a major merger.
