  With the help of the AdS/CFT correspondence, we easily derive the desired
response function of QFT on the boundary. Using the virtual optical system with
a convex lens, we are able to obtain the image of the black hole from the
response function and further study the Einstein ring of the non-commutative
black holes. All the results show that there are some common features and
different features compared to the previous study of other background black
holes. And with the change of the observation position, this ring will change
into a luminosity-deformed ring, or light points. In addition to these
similarities, there are some different features which are due to the
singularity of the event horizon temperature. Explicitly, the relation between
temperature and the event horizon $T-z_h$ has two branches when the
non-commutative parameter $n$ is fixed. These in turn have an effect on the
behavior of the response function and the Einstein ring. However, the amplitude
of $|\langle O\rangle|$ increases with the decrease of the temperature $T$ for
the left branch of $T-z_h$ relation, while the amplitude of $|\langle
O\rangle|$ decreases with the decrease of the temperature $T$ for the right
branch. These differences are also reflected in the Einstein ring. Therefore,
these differences can be used to distinguish different black hole backgrounds.
Furthermore, we show that the non-commutative parameter has an effect on the
brightness and the position of Einstein ring.
