  We report the spectral analysis of accretion powered millisecond X-ray pulsar
SAX J1748.9-2021 from the NuSTAR observation made during its 2015 outburst. The
spectra displayed a broad emission line at $\sim 6.5$ keV with line width of
$\sim 0.5$ keV and excess above $\sim 20$ keV due to Compton hump. The
persistent emission of SAX J1748.9-2021 is described by a combination of soft
thermal component with $kT =0.62^{+0.03}_{-0.05}$ keV and thermally Comptonized
component with $kT_e=2.50^{+0.06}_{-0.03}$ keV reflected from the disc with
reflection fraction of $0.30^{+0.08}_{-0.04}$. We have modeled the reflection
spectrum with self-consistent model relxillCP and have found the inclination of
the accretion disc to be $32.3^{^\circ +4.8}_{-4.7}$ and log $\xi$ is equal to
$3.05^{+0.40}_{-0.34}$. We have obtained an upper limit of 57 km for inner disc
radius; and the estimated magnetic field strength at the poles is less than
$3.4 \times 10^9$ G. This kind of detailed investigation of reflection spectrum
of SAX J1748.9-2021, especially above 10 keV, has been achieved only because of
high statistics NuSTAR data of the source.
