The observed galaxy exhibits a prominent disk structure with well-defined spiral arms. These arms appear somewhat loosely wound, extending outward from a central bulge. The bulge is moderately sized. The galaxy displays an overall blue hue in its spiral arms, indicative of ongoing star formation. A redder color is evident in the central bulge. There is a slight irregular morphology in the outer regions of the disk suggesting possible gravitational interaction. There is no apparent bar structure. There are 1-2 spiral arms visible. 