Observed (top), modeled (center), and model subtracted images (bottom) in the F606W (left), the F814W (center), and the F110W (right) HST filters using the final model derived in this paper. The images have been rotated, so that the major axis of the disk is oriented along the x-axis. Only the considered parts of the images are shown, while regions of large residuals from PSF subtraction or contaminated by other objects on the line of sight are masked. In the F606W and F814W images the ring-like structure of the disk is well reproduced by the model, and only the residuals from PSF subtraction of the central star remain visible. In the residual F110W image parts of the disk remain visible in the residual image suggesting that scattering at this wavelength is underestimated in the model. Note the different flux scales in different columns. The model image in the right column is displayed in a different way than the data and model subtracted data to better visualize the disk.