  NGC 4945 harbors one of the nearest active galactic nuclei (AGN), which
allows reaching high spatial resolution with the current observational
facilities. The Seyfert 2 nucleus is deeply obscured by an edge-on disk with
$A_V\sim14$, requiring infrared observations to study circumnuclear structures
and the interstellar medium. In this work, we present an imaging and longslit
spectroscopic study of the nuclear region with a spatial resolution of 6.5 pc,
based on Flamingos-2 (F2) and T-ReCS data taken at the Gemini South
observatory. We report sub-arcsecond photometric measurements of the nucleus in
$J$, $H$ and $K_{\rm s}$ filters, and at larger apertures. We do not detect
nuclear variability. The nuclear spectra confirm that even in $K$-band the AGN
emission-line features are completely obscured by dust. We detect a
circumnuclear disk in $K$-band as well as in the mid-infrared (MIR) $N$- and
$Q_{\rm a}$-bands, with a radial scale length of $\sim$120 pc. The disk shows
knots mostly in a ring-like arrangement that has been previously detected with
HST Pa $\alpha$ observations, indicating that these are deeply embedded,
massive young star clusters. We present here the spectrum of one of the
brightest and unresolved object (R$<5$pc), which we identify as a super star
cluster candidate with M$_{K_{\rm s}} -16.6\pm0.4$. For the circumnuclear
region, a detailed rotation curve allows to measure a nuclear mass of $M=(4.4
\pm 3)\times 10^{6} M_\odot$ within a radius of $\sim6.5$ pc. We also report
the detection of hot dust ($\sim 1000$ K) out to a nuclear distance of 80 pc
measured along the semi-major axis.
