  This work focuses on the examination of a regular black hole within
Verlinde's emergent gravity, specifically investigating the Hayward-like
(modified) solution. The study reveals the existence of three horizons under
certain conditions, i.e., an event horizon and two Couchy horizons. Our results
indicate regions which phase transitions occur based on the analysis of heat
capacity and Hawking temperature. To compute the latter quantity, we utilize
three distinct methods: the surface gravity approach, Hawking radiation, and
the application of the first law of thermodynamics. In the case of the latter
approach, it is imperative to introduce a correction to ensure the preservation
of the Bekenstein-Hawking area law. Geodesic trajectories and critical orbits
(photon spheres) are calculated, highlighting the presence of three light
rings. Additionally, we investigate the black hole shadows. Furthermore, the
quasinormal modes are explored using third- and sixth-order WKB approximations.
In particular, we observe stable and unstable oscillations for certain
frequencies. Finally, in order to comprehend the phenomena of time-dependent
scattering in this scenario, we provide an investigation of the time-domain
solution.
