  We present phase-resolved spectroscopy, photometry and circular
spectropolarimetry of the eclipsing polar UZ Fornacis. Doppler tomography of
the strongest emission lines using the inside-out projection revealed the
presence of three emission regions: from the irradiated face of the secondary
star, the ballistic stream and the threading region, and the magnetically
confined accretion stream. The total intensity spectrum shows broad emission
features and a continuum that rises in the blue. The circularly polarized
spectrum shows the presence of three cyclotron emission harmonics at $\sim$4500
\AA{}, 6000 \AA{} and 7700 \AA{}, corresponding to harmonic numbers 4, 3, and
2, respectively. These features are dominant before the eclipse and disappear
after the eclipse. The harmonics are consistent with a magnetic field strength
of $\sim$57 MG. We also present phase-resolved circular and linear
photopolarimetry to complement the spectropolarimetry around the times of
eclipse. MeerKAT radio observations show a faint source which has a peak flux
density of 30.7 $\pm$ 5.4 $\mu$Jy/beam at 1.28 GHz at the position of UZ For.
