Spatial distributions of diffuse sources around VCC 2095, one of the most edge‐on galaxies in our sample. Sources are divided by color at ﹩( g-z) _{0}=1.0﹩. Red sources (left) are generally in excess of the background, while blue sources (right) are consistent with background levels seen in control fields. The red sources are spatially clustered around the disk of the galaxy, supporting the idea that they are intrinsic to the galaxy. Blue sources are scattered more randomly through the field.