The 2.12 μm image of two separate systems of H₂ knots. HOD07 2 at 6^h7^m30.5^s, −6°11^{﹩\arcmin﹩}51^{﹩\arcsec﹩} is likely a small jet with several internal shocks. The bow shock HOD07 3 is located at 6^h7^m31.6^s, −6°12^{﹩\arcmin﹩}47^{﹩\arcsec﹩}. Projecting back from the bow shock along its plausible jet axis, we find a string of faint, slightly extended knots of emission that are also visible on the Spitzer 4.5 μm image. These faint emission features, indicated by arrows, are located at 6^h7^m33.2^s, −6°13^{﹩\arcmin﹩}03^{﹩\arcsec﹩}, at 6^h7^m34.1^s, −6°13^{﹩\arcmin﹩}24^{﹩\arcsec﹩}, and at 6^h7^m39.3^s, −6°14^{﹩\arcmin﹩}01^{﹩\arcsec﹩}. Overall, they appear to form a jet with multiple, faint internal shocks, ending in the bright bow shock.