The galaxy exhibits a spiral morphology, characterized by prominent, well-defined spiral arms. These arms appear to emanate from a central bulge region and extend outwards, tracing a loosely wound pattern. The color of the spiral arms suggest the presence of ongoing star formation. A bar-like structure may be present within the central region. The bulge exhibits a moderate size relative to the overall galactic structure. The disk of the galaxy is oriented close to face-on, showing no signs of significant interaction or major disturbances.
