Inclined ultra-diffuse galaxy AGC 242019. Left panel: Observed circular velocities (points with error bars) are well reproduced by MOND (solid black line) using the Newtonian contributions of stars (red dashed line) and gas (blue dotted line). Right panel: Corner plot showing the posterior distribution of the nuisance parameters. MOND predicts a distance of 12.5 Mpc, which is consistent with Virgocentric flow models.