We present VLA radio and Chandra X-ray observations of the merging galaxy cluster ( catalog Abell~3411 ) .
For the cluster , we find an overall temperature of 6.4 ^ { +0.6 } _ { -1.0 } keV and an X-ray luminosity of 2.8 \pm 0.1 \times 10 ^ { 44 } erg s ^ { -1 } between 0.5 and 2.0 keV .
The Chandra observation reveals the cluster to be undergoing a merger event .
The VLA observations show the presence of large-scale diffuse emission in the central region of the cluster , which we classify as a 0.9 Mpc size radio halo .
In addition , a complex region of diffuse , polarized emission is found in the southeastern outskirts of the cluster , along the projected merger axis of the system .
We classify this region of diffuse emission as a radio relic .
The total extent of this radio relic is 1.9 Mpc .
For the combined emission in the cluster region , we find a radio spectral index of -1.0 \pm 0.1 between 74 MHz and 1.4 GHz .
The morphology of the radio relic is peculiar , as the relic is broken up into five fragments .
This suggests that the shock responsible for the relic has been broken up due to interaction with a large-scale galaxy filament connected to the cluster or other substructures in the ICM .
Alternatively , the complex morphology reflects the presence of electrons in fossil radio bubbles that are re-accelerated by a shock .