The galaxy presents as a spiral type with prominent, well-defined spiral arms. The arms exhibit a moderate winding, not tightly wound nor exceptionally loose. A significant portion of the galaxy's light is concentrated in a moderately sized central bulge that appears yellowish. The arms are primarily bluish, suggesting active star formation regions. The galaxy disk is oriented close to face-on. There is no obvious indication of a strong central bar. The overall morphology appears relatively undisturbed, lacking obvious signs of a recent major merger, though minor disturbances cannot be ruled out based on the current image resolution.
