  In this paper, we discuss the possible effects of dark matter on a
Schwarzschild black hole with the correction of extended uncertainty principle
(EUP), such as the parameter $\alpha$ and the large fundamental length scale
$L_*$. In particular, we surround the EUP black hole of mass $m$ with a static
spherical shell of dark matter described by the parameters mass $M$, inner
radius $r_s$, and thickness $\Delta r_s$. In this study, we find that there is
no deviation in the event horizon, which readily implies that the black hole
temperature due to the Hawking radiation is independent of any dark matter
concentration. In addition, we show some effects of the EUP parameter on the
innermost stable circular orbit (ISCO) radius of time-like particles, photon
sphere, shadow radius, and weak deflection angle. It is found that time-like
orbits are affected by deviation of low values of mass $M$. A greater dark
matter density is needed to have remarkable effects on the null orbits. Using
the analytic expression for the shadow radius and the approximation $\Delta
r_s>>r_s$, it is revealed that $L_*$ should not be lower than $2m$. To broaden
the scope of this study, we also calculate the analytic expression for the weak
deflection angle using the Ishihara et al. method \cite{Ishihara_2016}. As a
result, we show that $\Delta r_s$ is improved by a factor of $(1+4\alpha
m^2/L_*^2)$ due to the EUP correction parameters. The calculated shadow radius
and weak deflection angle are then compared using the estimated values of the
galactic mass from Sgr A*, M87, and UGC 7232, as well as the mass of the
supermassive black hole at their center.
