  The first TeV gamma-ray source with no lower energy counterparts, TeV
J2032+4130, was discovered by HEGRA. It appears in the third HAWC catalog as
3HWC J2031+415 and it is a bright TeV gamma-ray source whose emission has
previously been resolved as 2 sources: HAWC J2031+415 and HAWC J2030+409. While
HAWC J2030+409 has since been associated with the \emph{Fermi-LAT} Cygnus
Cocoon, no such association for HAWC J2031+415 has yet been found. In this
work, we investigate the spectrum and energy-dependent morphology of HAWC
J2031+415. We associate HAWC J2031+415 with the pulsar PSR J2032+4127 and
perform a combined multi-wavelength analysis using radio, X-ray, and
$\gamma$-ray emission. We conclude that HAWC J2031+415 and, by extension, TeV
J2032+4130 are most probably a pulsar wind nebula (PWN) powered by PSR
J2032+4127.
