  We analyze 330 ks of {\it Chandra} X-ray imaging and spectra of the nearby,
edge-on starburst and Seyfert Type 2 galaxy NGC 4945 to measure the hot gas
properties along the galactic outflows. We extract and model spectra from 15
regions extending from $-$0.55 kpc to $+$0.85 kpc above and below the galactic
disk to determine the best-fit parameters and metal abundances. We find that
the hot gas temperatures and number densities peak in the central regions and
decrease along the outflows. These profiles are inconsistent with a spherical,
adiabatically-expanding wind model, suggesting the need to include mass loading
and/or a non-spherical outflow geometry. We estimate the mass outflow rate of
the hot wind to be $1.6\:M_{\odot}~\rm{yr}^{-1}$. Emission from charge exchange
is detected in the northern outflow, and we estimate it contributes 12\% to the
emitted, broad-band ($0.5-7$ keV) X-ray flux.
