  This study focuses on investigating a regular black hole within the framework
of Verlinde's emergent gravity. In particular, we explore the main aspects of
the modified Simpson--Visser solution. Our analysis reveals the presence of a
unique physical event horizon under certain conditions. Moreover, we study the
thermodynamic properties, including the Hawking temperature, the entropy, and
the heat capacity. Based on these quantities, our results indicate several
phase transitions. Geodesic trajectories for photon-like particles,
encompassing photon spheres and the formation of black hole shadows, are also
calculated to comprehend the behavior of light in the vicinity of the black
hole. Additionally, we also provide the calculation of the time delay and the
deflection angle. Corroborating our results, we include an additional
application in the context of high-energy astrophysical phenomena: neutrino
energy deposition. Finally, we investigate the quasinormal modes using
third-order WKB approximation.
