The galaxy appears as a face-on spiral galaxy, exhibiting a moderately sized central bulge. The spiral arms are relatively tightly wound, suggesting a grand-design spiral structure. There are likely multiple spiral arms, more specifically two, that wind outward. The blueness in the arms may indicate ongoing star formation regions. The central bulge appears yellowish, possibly indicating an older stellar population. The galaxy doesn't show strong evidence of a bar feature. There is also no evidence of any major mergers occurring. The overall appearance suggests a spiral galaxy undergoing relatively normal evolution with a moderate amount of star formation activity in the disk, and a more quiescent bulge.
