The galaxy exhibits a distinct spiral structure. Two prominent spiral arms emanate from a central bulge, displaying a moderate winding. The arms show a clumpy texture suggestive of active star formation regions. The central bulge appears moderate in size, transitioning smoothly into the spiral disk. The galaxy is observed face-on, allowing for a clear view of its spiral morphology. The disk shows a blueish hue, contrasting with the more yellowish central bulge. The overall structure appears relatively undisturbed, with no obvious signs of recent major merger events. A weak bar may be present within the central region.
