  SXP 1323 is a peculiar high-mass X-ray binary located in the Small Magellanic
Cloud, renowned for its rapid spin-up. We investigate for the first time
broadband X-ray properties of SXP1323, as observed by the Mikhail Pavlinsky
ART-XC and eRosita telescopes on board the SRG observatory. Using ART-XC and
eRosita, data we produced first broadband 1-20 keV X-ray spectrum and estimated
pulsed fraction above 8 keV. With the addition of archival XMM-Newton
observations we traced evolution of the SXP 1323 spin period over the last five
years and found that after 2016 the source switched to a linear spin-up with
rate of -29.9 s yr$^{-1}$. Broadband X-ray spectrum is typical for accreting
X-ray pulsars, with steep powerlaw index ($\Gamma$=-0.15) and exponential
cutoff energy of 5.1 keV. No significant difference between spectra obtained in
states with and without pulsations were found.
