  By utilizing the AdS/CFT correspondence, we investigate the holographic image
of an AdS black hole in Einstein-power-Yang-Mills gravity. The AdS boundary
hosts a Gaussian oscillation source, which induces a lensed response on the
opposite side of the boundary during propagation through bulk spacetime. The
optical system assists observers at the north pole to continuously capture
holographic images that show an axisymmetric bright ring known as the Einstein
ring. As the observation position shifted, the bright ring gradually
transformed into a luminous arc and eventually transitioned into a light point.
Simultaneously, we examine the impact of variations in relevant physical
quantity on the ring, and present the corresponding brightness curve. The
results indicate that as the temperature $T$ and nonlinear Yang Mills charge
parameter $q$ increase, the ring radius also increases, while an increase in
the chemical potential $u$ leads to a decrease. However, the peak brightness
curve of the ring invariably decreases as the values of $T$, $u$, and $q$
increase, albeit to varying degrees. Upon comparing the outcomes of geometric
optics, it can be observed that the position of the ring in holography images
is consistent with that of the photon sphere.
