The galaxy presents as a face-on spiral galaxy, with a moderate-sized bulge relative to the disk. The disk exhibits a dominant, well-defined two-arm spiral structure, demonstrating a winding pattern that appears to be intermediate between tightly wound and loosely wound. The arms show evidence of active star formation. There are no obvious signs of a strong central bar structure. Overall, the morphology suggests a relatively undisturbed spiral galaxy, though minor disturbances cannot be ruled out. The color profile indicates a redder hue, suggesting an older stellar population within the bulge.
