The galaxy M106 is about 31Mly away and is also known as NGC4258.  The supermassive black hole near its center is surrounded by a disk of accreting matter that generates enormous energy especially at ultraviolet and x-ray wavelengths, thought to be related to but dimmer than distant quasars.  

This image was processed using PixInsight and noise reduction techniques as taught by Jon Rista resulting in preserving many other interesting features.  Some of these features were galaxies and quasars down to about 21st magnitude and at distances of 8.6 Bly and 13.2 Bly respectively.  Most of the distant objects are quasars unless otherwise marked or obviously seen as galaxies in the image (if it's "fuzzy" think galaxy, if it's a a well defined dot think quasar unless the annotation says otherwise). 

The ImageSolver and AnnotateImage scripts in PixInsight were used to indicate some galaxies as far away as 2 Bly as shown in turquoise color.  I then manually determined the distances and annotated in white color other distant objects by using www.aladin.u-strasbg.fr/AladinLite/ as a planetarium program and selecting the Sloan Digital Sky Survey 9 (SDSS9) as sky image and the SIMBAD catalogue.  I carefully matched SIMBAD hits with my image data to determine the annotation positions of selected distant objects between "- -" marks.  For each selected object I converted the reported radial velocity (radvel) in km/s to distance by dividing the radvel by the Hubble constant H0 = 67.8 km/s/Mpc and then converting Mpc to Mly.  These distances are simplistic since I'm not prepared to get into discussions about the curvature of space-time but are consistent insofar as close galaxies are generally bigger and brighter than distant ones.  I also found two pulsars and annotated them in turquoise since they are within the Milky Way. 

In the image, the farthest objects are little more than faint accumulations of a few pixels rising out of the background noise but definitely "there," so you may need to zoom in by left clicking and dragging on the image to see those captured photons from near the beginning of this universe.