The galaxy presents a disk-like structure, viewed approximately face-on. Spiral arm structures appear present, with some arms appearing more tightly wound than others. The central bulge is prominent, displaying a significant concentration of light and contributing substantially to the overall luminosity. The bulge appears moderately sized relative to the galactic disk. There's evidence of a bar-like feature traversing the central region. The galaxy doesn't show strong indications of major mergers, but slight asymmetries suggest possible minor disturbances. The disk exhibits areas of active star formation, indicated by the blueish tint within the spiral arms.
