  Moderate resolution spectra of four globular clusters in the dwarf spheroidal
galaxy IKN obtained with the 6-m telescope of the Special Astrophysical
Observatory have been used to determine the radial velocities, ages, and
metallicities of the clusters, and also to derive the first approximate
estimates of the abundances of Mg, Ca, and C. Cross-correlation with
radial-velocity standards, fitting of the observed spectra with model spectra,
diagnostic diagrams based on the Lick absorption indices, and comparison of the
spectra and absorption indices with those of Galactic globular clusters are
applied. The integrated-light (IL) spectrum of the two bright clusters IKN4 and
IKN5, which are close to the center of the galaxy in projection on the
celestial sphere, yields the heliocentric radial velocity $V_h= 38\pm30$ km/s,
age $T=12.6\pm2$ Gyr, metallicity $[Fe/H]=-2.1\pm0.2$ dex and abundance of
$\alpha$-process elements $[\alpha/Fe] \sim 0.5$ dex. The IL spectrum of the
two weaker clusters IKN1 and IKN3, which are far from the center of the galaxy,
yields the radial velocity $V_h=-39 \pm 50$ km/s. Despite of the low signal to
noise ratio in the summary spectrum of IKN1 and IKN3, one can conclude from the
comparison of the results of different used methods, that IKN1 and IKN3 have
seemingly the same age and metallicity as IKN4 and IKN5. According to the
measured Lick indices H$_{\delta_{\rm F}}$ and H$_{\beta}$, the studied
globular clusters in IKN have blue horizontal branches.
