  We present results from the James Webb Space Telescope (JWST) Director's
Discretionary Time Early Release Science (ERS) program 1328 targeting the
nearby, Luminous Infrared Galaxy (LIRG), VV 114. We use the MIRI and NIRSpec
instruments to obtain integral-field spectroscopy of the heavily obscured
Eastern nucleus (V114E) and surrounding regions. The spatially resolved,
high-resolution, spectra reveal the physical conditions in the gas and dust
over a projected area of 2-3 kpc that includes the two brightest IR sources,
the NE and SW cores. Our observations show for the first time spectroscopic
evidence that the SW core hosts an AGN as evidenced by its very low 6.2 {\mu}m
and 3.3 {\mu}m PAH equivalent widths (0.12 and 0.017 {\mu}m respectively) and
mid and near-IR colors. Our observations of the NE core show signs of deeply
embedded star formation including absorption features due to aliphatic
hydrocarbons, large quantities of amorphous silicates, as well as HCN due to
cool gas along the line of sight. We detect elevated [Fe II]/Pf{\alpha}
consistent with extended shocks coincident with enhanced emission from warm
H$_{2}$, far from the IR-bright cores and clumps. We also identify broadening
and multiple kinematic components in both H$_{2}$ and fine structure lines
caused by outflows and previously identified tidal features.
