The galaxy presents as a face-on spiral, exhibiting a clear disk structure with defined spiral arms. Two prominent arms extend from the central region, winding moderately tightly around the bulge. The central bulge appears moderate in size and exhibits a yellow hue, potentially indicating an older stellar population. The spiral arms show signs of ongoing star formation, indicated by bluer regions within the disk. There is no clear sign of a strong bar feature, but perhaps a weak one. The overall structure suggests a relatively undisturbed system, though there might be some minor disturbances in the spiral arm structure.
