Motivated by the recent discovery of superconductivity in LaNiO under pressure, we discuss the basic ingredients of a model that captures its microscopic physics under pressure tuning. We anchor our description in terms of the spectroscopic evidence of strong correlations in this system. In a bilayer Hubbard model including the Ni and orbitals, we show the ground state of the model crosses over from a low-spin state to a high-spin state. In the high-spin state, the two and the bonding orbitals are all close to half-filling, which promotes a strong orbital selectivity in a broad crossover regime of the phase diagram pertinent to the system. Based on these results, we construct an effective multiorbital - model to describe the superconductivity of the system, and find the leading pairing channel to be an intraorbital spin singlet with a competition between the extended -wave and symmetries. Our results highlight the role of strong multiorbital correlation effects in driving the superconductivity of LaNiO.

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