The galaxy presents as a spiral type, with a prominent disk structure. The arms are tightly wound around a central bulge, exhibiting a relatively smooth texture, with a small degree of clumpiness, suggesting a moderate level of star formation. There appears to be a weak bar structure extending through the bulge region. The bulge is relatively small in comparison to the overall size of the galaxy, and appears to have a strong concentration. The blue coloration in the spiral arms suggests the presence of young, hot stars. The galaxy appears nearly face-on, allowing for a good view of the spiral arm structure. There seems to be little to no evidence of interactions or mergers disturbing its overall morphology. 
