The galaxy exhibits a distinct spiral morphology, viewed at a slight angle relative to edge-on. The arms are tightly wound, indicating potentially an Sa or Sab classification. A central bulge is apparent, but appears small relative to the overall disk size. The disk shows clear signs of star formation, evidenced by the bluish color. There does not appear to be any strong evidence of a bar structure, and the image quality indicates a lack of interactions or major disturbances.
