The galaxy presents a distinct spiral morphology. The disk component dominates the overall structure, exhibiting well-defined spiral arms. These arms are tightly wound, tracing a relatively compact pattern around the galactic center. The winding tightness suggests a possible connection to a higher rate of shear within the disk. A small bulge is visible, with moderate luminosity compared to the disk. The arms feature a mottled appearance with knots of brighter regions indicative of active star formation. The galaxy exhibits a bluish hue, consistent with ongoing stellar formation activity. The morphology suggests that the galaxy has not experienced a recent major merger, though signs of possible minor interactions cannot be fully excluded based solely on the morphology of the galaxy presented.
