Abstract I report the discovery of a stellar stream (Sutlej) using Gaia DR3 proper motions and XP metallicities located ∼15○ north of the Small Magellanic Cloud (SMC). The stream is composed of two parallel linear components (“branches”) approximately ∼8○ × 0.6○ in size and separated by 2.5○. The stars have a mean proper motion of (μRA, μDEC)=(+0.08 mas yr−1,−1.41 mas yr−1) which is quite similar to the proper motion of stars on the western side of the SMC. The color magnitude diagram of the stream stars has a clear red giant branch, horizontal branch, and main sequence turnoff that is well-matched by a PARSEC isochrone of 10 Gyr, [Fe/H]=−1.8 at 32 kpc and a total stellar mass of ∼33,000 M⊙. The stream is spread out over an area of 9.6 square degrees and has a surface brightness of 32.5 mag arcsec−2. The metallicity of the stream stars from Gaia XP spectra extend over −2.5 ≤ [M/H] ≤ −1.0 with a median of [M/H]=−1.8. The tangential velocity of the stream stars is 214 km s−1 compared to the values of 448 km s−1 for the Large Magellanic Cloud and 428 km s−1 for the SMC. While the radial velocity of the stream is not yet known, a comparison of the space velocities using a range of assumed radial velocities, shows that the stream is unlikely to be associated with the Magellanic Clouds. The tangential velocity vector is misaligned with the stream by nearly 90○, which might indicate an important gravitational influence from the nearby Magellanic Clouds.