As stated in a previous answer, the photon emitted in a radial direction will not come back to the black hole and will move away in the same direction with speed $ c $ to infinity, with a decreasing measured frequency.
This can be completed with the effect of general relativity on the photon geodesic which will be different from that of classical mechanics.
Applying the Schwarzschild metric to an outgoing geodesic $ \frac{dr}{dt}>0 $, it is written as:
$$ ct=r+R_s\ln{(\frac{r}{R_s}-1)}+constant\ \ \ \ \ [A]$$
with $ r $ radial coordinate of the photon, $ c $ speed of the light in vacuum and $ R_s $ Schwarzschild radius $ = \frac{2GM}{c^2} $.
When $ r\gg R_s $, the logarithm term is negligible and $ [A] $ turns into:
$$ ct\simeq r+constant $$
which is the equation for radial light beams in a flat space-time (classical mechanics).
In the hope of having usefully completed the answer,
Best regards.