The galaxy exhibits a defined spiral structure, with discernible arms extending from a central bulge. These spiral arms appear relatively tightly wound. The central bulge has a moderate size, and shows an elongated shape. The galaxy's disk appears close to face-on. Color gradients suggest regions of active star formation within the arms. There is also evidence of a bar-like structure crossing the bulge. No significant morphological disturbance or signs of a recent major merger are clearly visible.
