The galaxy presents a distinct spiral morphology. Prominent, well-defined spiral arms emanate from a central bulge. The arms exhibit a clumpy structure, suggestive of active star formation regions, interspersed with dust lanes that trace the spiral pattern. The bulge appears relatively small and exhibits a smooth, yellowish color, potentially indicating an older stellar population. The disk of the galaxy is visible and appears more extended than the bulge. There is no obvious central bar structure visible. The galaxy appears relatively isolated, showing no signs of major ongoing merging activity, although there may be a minor disturbance of some sort. Overall, the galaxy appears to be a late-type spiral galaxy with significant star formation activity within its spiral arms.
