The galaxy presents a spiral structure, although the arms are not tightly wound and appear somewhat flocculent. A central bulge is visible, contributing significantly to the overall luminosity of the galaxy. The disk exhibits a blue hue, suggesting the presence of younger stellar populations and ongoing star formation. There is no evidence of a strong bar feature bisecting the bulge, although a subtle asymmetry could indicate a weak bar. The morphology appears relatively undisturbed, with no signs of significant tidal interactions or major mergers. The galaxy's colour profile transitions smoothly from the inner bulge to the outer disk, with the bluer regions concentrated in the spiral arms. The overall appearance suggests a galaxy that is not experiencing extreme starburst activity, but maintains a steady rate of star formation. 
