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Many ultra diffuse galaxies (UDGs) have now been identified in clusters ofgalaxies. However, the number of nearby UDGs suitable for detailed follow-upremain rare. Our aim is to begin to identify UDGs in the environments of nearbybright early-type galaxies from the VEGAS survey. Here we use a deep g bandimage of the NGC 5846 group, taken as part of the VEGAS survey, to search forUDGs. We found one object with properties of a UDG if it associated with theNGC 5846 group, which seems likely. The galaxy, we name NGC 5846$\_$UDG1, hasan absolute magnitude of M$_g$ = -14.2, corresponding to a stellar mass of$\sim$10$^8$ M$_{\odot}$. It also reveals a system of compact sources which arelikely globular clusters. Based on the number of globular clusters detected weestimate a halo mass that is greater than 8$\times$10$^{10}$ M$_{\odot}$ forUDG1.

An Ultra diffuse Galaxy in the NGC 5846 group from the VEGAS survey