The galaxy exhibits a distinct spiral morphology. The arms appear loosely wound and extend outwards from a central region that shows signs of a small bulge. The overall color suggests active star formation, particularly within the spiral arms, which display a bluish hue. The presence of star formation regions appears prominent. The galaxy does not appear significantly distorted, but there might be a slight asymmetry in the arm structure, possibly indicative of a minor gravitational interaction or internal dynamic process. It is likely a disk galaxy, and does not appear to be merging. A very faint bar structure is present.