A regular black hole with a de Sitter core would oscillate at slightly different frequencies, transmit less Hawking radiation, evaporate more slowly, and cast a slightly smaller, dimmer shadow than a Schwarzschild black hole of the same mass.
Conditions for the oc- curence of strong curvature singularities.Journal of Geometry and Physics, 2(2):127–143
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Signatures of a de Sitter-core black hole in ringing, transmission and optical appearance
A regular black hole with a de Sitter core would oscillate at slightly different frequencies, transmit less Hawking radiation, evaporate more slowly, and cast a slightly smaller, dimmer shadow than a Schwarzschild black hole of the same mass.