The observed galaxy presents as a spiral galaxy with a significant central bulge. The bulge appears yellowish-white, suggesting an older stellar population with a lower rate of star formation compared to the disk. Distinct spiral arms emanate from the central region. These spiral arms are traced by regions of blue light, suggestive of recent or ongoing star formation. Dust lanes may be present along the inner edges of the arms, obscuring some of the light. The galaxy is not perfectly face-on, presenting a slightly inclined disk. The structure appears largely undisturbed, showing no obvious signs of a major merger. A weak bar may be present. The spiral arms exhibit an intermediate winding. The number of spiral arms is most likely two.
