When some stars reach the end of their lives they explode as a supernova (SN), and the ejecta from the progenitor star forms an expanding structure known as a supernova remnant (SNR). We currently know of around 300 SNRs in our Galaxy, however current models predict there should be closer to 1500 observable SNRs. This deficit is attributed to present-day observational challenges and new discoveries are necessary to bridge this knowledge gap. Smeaton et al. add to this list by presenting a new Galactic SNR candidate G312.65+2.87, dubbed Unicycle. Based primarily on its radio morphology, the source is identified as a possible Galactic shell-type SNR candidate. The radio shell has a size of 288 arcseconds × 300 arcseconds. Unicycle displays a large degree of circularity which may indicate it as the remnant of a Type Ia supernova. Wide-Field Infrared Survey Explorer (WISE) survey images at wavelengths of 3.4, 4.6, 12, and 22 μm revealed no obvious corresponding infrared emission. This indicates the radio emission from Unicycle is likely caused by synchrotron emission. For shell-type SNRs, this synchrotron emission is generated by the relativistic particles in the expanding shock front. The image above is an RGB composite image where the 944 MHz ASKAP image is in red and blue and WISE 12 μm infrared image is in green.