If you know of such a relation, please post a reference paper.
Not directly, because these two quantities are not known to correlate as strongly as other "intermediate" relations. But they do correlate, with bigger disks in bigger haloes; it's fairly intuitive.
You could construct a relation from e.g. The Luminosity-Size and Mass-Size Relations of Galaxies out to z ~ 3 (or more specific to B-band, but more simulation focused Interpreting the Evolution of the Size - Luminosity Relation for Disk Galaxies from Redshift 1 to the Present) and Constraints on the Relationship between Stellar Mass and Halo Mass at Low and High Redshift. The various forms of the Tully-Fisher relation may also be useful.