The galaxy presents a clear disk structure with well-defined spiral arms. These spiral arms are tightly wound, suggesting a relatively high shear rate within the galaxy. A central bulge is present, exhibiting a moderate size compared to the overall galactic disk. There is no apparent bar structure visible at this resolution. The galaxy is not observed edge-on. The spiral structure appears somewhat flocculent, without grand, sweeping arm features. Indications suggest that this is not a particularly massive galaxy, and it is currently undergoing a moderate level of star formation. There are features of possible minor disturbances to the arms of the galaxy, though no apparent signs of a major merger.