The rim of this crater is broken in the south and the interior is flooded with lava. The terrain about the crater has also been resurfaced by past lava flows, leaving on a low rim raised about the nearly level surroundings. The southwest rim is attached to a low rim that connects with da Vinci.
This crater was previously designated Taruntius D before being named by the IAU.
References
^"Watts (crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
Andersson, L. E.; Whitaker, E. A. (1982). NASA Catalogue of Lunar Nomenclature. NASA RP-1097.
Menzel, D. H.; Minnaert, M.; Levin, B.; Dollfus, A.; Bell, B. (1971). "Report on Lunar Nomenclature by the Working Group of Commission 17 of the IAU". Space Science Reviews. 12 (2): 136–186. Bibcode:1971SSRv...12..136M. doi:10.1007/BF00171763. S2CID122125855.