We report the observation and physical characterization of the possible dwarf planet UZ (DeeDee), a dynamically detached trans-Neptunian object discovered at 92 AU. This object is currently the second-most distant known trans-Neptunian object with reported orbital elements, surpassed in distance only by the dwarf planet Eris. The object was discovered with an $r$-band magnitude of 23.0 in data collected by the Dark Energy Survey between 2014 and 2016. Its 1140-year orbit has $(a,e,i) = (109~mathrm{AU}, 0.65, 26.8^{circ})$. It will reach its perihelion distance of 38 AU in the year 2142. Integrations of its orbit show it to be dynamically stable on Gyr timescales, with only weak interactions with Neptune. We have performed followup observations with ALMA, using 3 hours of on-source integration time to measure the objects thermal emission in the Rayleigh-Jeans tail. The signal is detected at 7$sigma$ significance, from which we determine a $V$-band albedo of $13.1^{+3.3}_{-2.4}mathrm{(stat)}^{+2.0}_{-1.4}mathrm{(sys)}$ percent and a diameter of $635^{+57}_{-61}mathrm{(stat)}^{+32}_{-39}mathrm{(sys)}$~km, assuming a spherical body with uniform surface properties.
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