Model fits of the observational data for the near model. Top: the SED, where the aperture-corrected model flux levels are shown as crosses and the dotted line, and the observed flux values are shown as filled squares and the solid line. Middle: the modeled (lines) and observed (points) MIDI visibilities for three wavelengths. Bottom: the modeled (blue points) and observed (green points) radial intensity distributions from the Hi-GAL (70 and 160 μm) and ATLASGAL (870 μm) images.