The present study aims at characterizing the habitability conditions of exoplanets with an Earth-like magnetosphere inside the habitable zone of M and F stars, caused by the direct deposition of the stellar wind on the exoplanet surface. Also, the radio emission generated by exoplanets with a Earth-like magnetosphere is calculated for different space weather conditions. The study is based on a set of MHD simulations performed by the code PLUTO. Exoplanets hosted by M stars at $0.2$ au are protected from the stellar wind during regular and CME-like space weather conditions if the star rotation period is slower than $3$ days. Exoplanets hosted by a F stars at $\geq 2.5$ au are protected during regular space weather conditions, but a stronger magnetic field compared to the Earth is mandatory if the exoplanet is close to the inner edge of the star habitable zone ($2.5$ au) during CMEs. The range of radio emission values calculated in the simulations are consistent with the scaling proposed by \citeA{Zarka8} during regular and common CME-like space weather conditions. If the radio telescopes measure a relative low radio emission signal with small variability from an exoplanet, that may indicate favorable exoplanet habitability conditions. The radio emission power calculated for exoplanets with an Earth-like magnetosphere is in the range of $3 \cdot 10^{7}$ to $2 \cdot 10^{10}$ W for SW dynamic pressures between $1.5$ to $100$ nPa and IMF intensities between $50$ - $250$ nT, and is below the sensitivity threshold of present radio telescopes at parsec distances.