This galaxy presents a distinct spiral morphology. The central bulge is relatively small and exhibits a yellowish-white hue, suggesting an older stellar population. Prominent spiral arms extend outwards from the bulge, displaying a tightly wound structure. These arms are traced by regions of blue light indicative of ongoing star formation. There are at least two well-defined spiral arms that are dominant. A faint, elongated feature, possibly a weak bar, appears to be present in the central region of the galaxy. The overall color is dominated by blues, with regions of red present. This suggests a significant proportion of young, hot stars and ionized gas. The disk is viewed at a shallow angle. The galaxy doesn't present any signs of major merging activity, though minor disturbances can not be ruled out.
