Images showing the total polarized flux in the H filter (left) and K_s filter (right). The innermost saturated pixels were masked out and the images were convolved with a Gaussian kernel with a FWHM of 4 pixels (i.e., the FWHM of the PSF). While the H image is flux-calibrated, showing the flux in units of surface brightness, the unit of the K_s image is counts per pixel. North is up, east to the left.