The observed galaxy presents as a spiral galaxy, exhibiting well-defined spiral arms. The arms appear somewhat flocculent, displaying a moderate degree of winding. A discernible central bulge is evident, contributing significantly to the overall luminosity. A stellar bar may be present within the central region of the galaxy. The disk appears to be oriented close to face-on, allowing for clear visualization of its spiral structure. Star formation appears to be actively occurring within the spiral arms. The galaxy displays a blueish tint, suggesting the presence of young, hot stars. The galaxy is a reasonably large distance away from the observer. There is no obvious signs of major galactic interaction or merging events currently affecting its morphology.
