A 2.12 μm S(1) line + continuum image containing two separate systems of H₂ knots. The circle identifying HOD07 11 at 6^h7^m46.9^s, −6°20^{﹩\arcmin﹩}6^{﹩\arcsec﹩} marks the putative position of the central source of a jet extending to the north‐northeast (﹩\mathrm{P.A.}\,\approx 23^{\circ }﹩) and ending in a well‐defined bow shock located at 6^h7^m48.6^s, −6°19^{﹩\arcmin﹩}3^{﹩\arcsec﹩}. Several fainter knots of S(1) emission lie between the center and the bow shock, completing the morphology of a typical jet. HOD07 12 at 6^h7^m49.8^s, −6°20^{﹩\arcmin﹩}43^{﹩\arcsec﹩} has the morphology of a faint bipolar nebula. Two other knots of S(1) emission lie to the southeast at 6^h7^m51.6^s, −6°20^{﹩\arcmin﹩}58^{﹩\arcsec﹩} and at 6^h7^m54.9^s, −6°21^{﹩\arcmin﹩}57^{﹩\arcsec﹩}. While there are a number of faint features to the northeast of the bipolar nebula, no clear association with this jet source can be established.