The galaxy presents as a face-on spiral with two dominant, well-defined spiral arms. There are signs of ongoing star formation, with the arms exhibiting localized regions of bluish color, indicative of young, hot stars. The central bulge appears relatively small and indistinct compared to the overall disk, displaying a yellowish-white hue suggesting an older stellar population. No prominent bar feature is discernible. The spiral arms exhibit a tightly wound morphology, appearing close together and wrapping around the central bulge. There is no obvious indication of major interaction or merging events, but a few regions show minor disturbances in the spiral arm structure. The disk of the galaxy appears more prominent than the bulge, indicating a later-type spiral galaxy classification.
