The galaxy exhibits a prominent spiral structure with multiple, tightly wound arms emanating from a bright central bulge. The arms display variations in color and luminosity, suggesting differential stellar populations and star formation activity. The bulge region appears relatively smooth and concentrated. The galaxy's overall color suggests a mix of older stellar populations and ongoing star formation. No obvious signs of major mergers or strong tidal disturbances are readily apparent, although there is a slight asymmetry in the outer regions of the arms. The morphology appears to be a spiral galaxy, with a relatively small and moderately bright bulge, with a slight bar present. The galaxy is presented at an angle, allowing for the disk to be seen from an oblique view.
