  This work mainly focuses to unveil the optical features of a black hole. For
this objective, we utilize the metric-affine black hole geometry with the
inclusion of dilation, spin, and shear charge. The Lagrangian coefficients
$f_1$ and $d_1$ are the main parameters, where $f_1<0$, which differentiate the
solutions by $d_1=8f_1,\;d_1=-8f_1,\;\&\;d_1=\pm8f_1$. Based on these
parameters, we carry out this work in two cases, i.e.,
$d_1=8f_1,\;\&\;d_1=-8f_1$. We forecast the detailed impact of dilation, spin,
and shear charges on the optical properties of the black holes in both cases.
To unreveal the optical features, we calculate horizon radius, inner stable
circular orbit, photon sphere radius, BH shadows, quasi-periodic oscillations,
the red-blue shift of photon particles, effective force, weak gravitational
lensing, and image magnification by using metric-affine gravity black hole
geometry.
