The observed galaxy exhibits a clear spiral structure. Two prominent spiral arms emanate from a central bulge. The winding of these arms appears medium in tightness. A bar structure is present and appears moderately strong, bisecting the central bulge. The central bulge appears moderate in size relative to the overall galaxy. The disk is not edge-on. There's no visually apparent major merging activity. The galaxy exhibits a smooth overall appearance with prominent spiral features. The color gradient suggests a higher concentration of older stellar populations in the central bulge, with younger, bluer stars likely populating the spiral arms.
