  In this paper, we utilize recent observational data from Gamma-Ray Bursts
(GRBs) and Pantheon+ Supernovae Ia (SNe Ia) sample to explore the interacting
Dark Energy (IDE) model in a phenomenological scenario. Results from GRBs-only,
SNe Ia and GRBs+SNe Ia indicate that the energy is transferred from dark energy
to dark matter and the coincidence problem is alleviated. The value of H0 from
GRBs+SNe Ia in the IDE scenario shows agreement with the SH0ES measurement.
Considering the age estimate of the quasar APM 08279+5255 at z = 3.91, we find
that the phenomenological IDE scenario can predict a cosmic age greater than
that of the {\Lambda}CDM model, thus the cosmic age problem can be alleviated.
