  James Webb Space Telescope NIRCam images have revealed 154 reliable globular
cluster (GC) candidates around the $z = 0.0513$ elliptical galaxy VV~191a after
subtracting 34 likely interlopers from background galaxies inside our search
area. NIRCam broadband observations are made at 0.9-4.5 $\mu$m using the F090W,
F150W, F356W, and F444W filters. Using PSF-matched photometry, the data are
analyzed to present color-magnitude diagrams (CMDs) and color distributions
that suggest a relatively uniform population of GCs, except for small fractions
of reddest (5-8%) and bluest (2-4%) outliers. GC models in the F090W vs.
(F090-F150W) diagram fit the NIRCam data well and show that the majority of GCs
detected have a mass of approximately $\sim$$10^{6.5}$$M_{\odot}$, with
metallicities [Fe/H] spanning the typical range expected for GCs (-2.5$\le$
[Fe/H]$\le$ 0.5). However, the models predict $\sim$0.3-0.4 mag bluer
(F356W-F444W) colors than the NIRCam data for a reasonable range of GC ages,
metallicities, and reddening. Although our data does not quite reach the
luminosity function turnover, the measured luminosity function is consistent
with previous measurements, suggesting an estimated peak at $m_{\rm
AB}$$\sim$-9.4 mag, $\pm$0.2 mag in the F090W filter.
