This galaxy exhibits a distinct spiral morphology. Tightly wound spiral arms are visible, emanating from a central, relatively bright bulge. The galaxy is observed nearly face-on, allowing a clear view of its spiral structure. The central bulge appears yellowish, suggesting an older stellar population, while the spiral arms show a bluer hue, indicative of ongoing star formation. No significant bar structure is apparent. Overall, the galaxy appears to be in a relatively undisturbed state, without obvious signs of a major merger, although the galaxy may be undergoing minor disturbances.
