SHAPE mesh model of V605 Aql and comparison with its HST F502N image of the [O III] λ5007 Å emission line. Top-left: edge-on view of the SHAPE mesh model consisting of a molecular disk (green) and collimated outflows and ionized bipolar outflows (blue and red). The inclination angle of the disk with the plane of the sky is 63°, as derived from the best-fit model. Top-right: projection onto the plane of the sky of the SHAPE mesh model. For comparison the right panel of Fig. 5 in Tafoya et al. (2022) is shown in the upper right corner of this panel. Bottom: HST [O III] image (left) and synthetic image (right). The [O III] synthetic image is computed from the ionized bipolar outflows. The molecular disk does not contribute to the emission, but it rather absorbs the optical emission behind it, which is accounted for adopting an ad hoc emission law for the ionized material. We refer to Sect. 4.1 for details.