The galaxy presents as a spiral, displaying well-defined spiral arms that emanate from a central bulge. The spiral arms appear tightly wound around the central bulge, appearing as two dominant arms. The central bulge has a yellowish-orange hue, suggesting an older stellar population and a potential lower rate of star formation in that region. Moving outward from the bulge, the arms exhibit a bluer color, indicative of ongoing star formation. There is no visible bar structure. There are no clear signs of significant morphological disturbance or a major ongoing merger.
