  We present the discovery of highly-collimated radio jets spanning a total of
355 kpc around the nearby elliptical galaxy NGC 2663, and the possible first
detection of recollimation on kiloparsec scales. The small distance to the
galaxy (~28.5 Mpc) allows us to resolve portions of the jets to examine their
structure. We combine multiwavelength data: radio observations by the Murchison
Widefield Array (MWA), the Australian Square Kilometre Array Pathfinder (ASKAP)
and the Australia Telescope Compact Array (ATCA), and X-ray data from Chandra,
Swift and SRG/eROSITA. We present intensity, rotation measure, polarisation,
spectral index and X-ray environment maps. Regions of the southern jet show
simultaneous narrowing and brightening, which can be interpreted as a signature
of the recollimation of the jet by external, environmental pressure, though it
is also consistent with an intermittent Active Galactic Nuclei (AGN) or complex
internal jet structure. X-ray data suggest that the environment is extremely
poor; if the jet is indeed recollimating, the large recollimation scale (40
kpc) is consistent with a slow jet in a low-density environment.
