NGC 4707 is an irregular galaxy in the constellation of Canes Venatici. It was discovered by John Herschel on 5 June 1834,^[4] and was described by John Louis Emil Dreyer, the compiler of the New General Catalogue, as a "small, stellar" galaxy.^[5]

NGC 4707
NGC 4707, imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
Constellation	Canes Venatici
Right ascension	12h 48m 21.666s[1]
Declination	+51° 09′ 53.81″[1]
Redshift	0.001561[2]
Heliocentric radial velocity	468 km/s[2]
Distance	22.11 ± 3.64 Mly (6.780 ± 1.116 Mpc)[2]
Apparent magnitude (V)	12.91[2]
Apparent magnitude (B)	15.2[3]
Absolute magnitude (V)	-16.23[2]
Characteristics
Type	Sm/Im[3]
Size	16,100 ly (4,930 pc)[2]
Apparent size (V)	1.120′ × 1.045′[3]
Other designations
UGC 7971, MCG+09-21-050, PGC 43255, DDO 150[3]

NGC 4707 has a morphological type of Sm or Im, meaning that it is mostly irregular or has very weak spiral arms.^[3] The galaxy was imaged by the Hubble Space Telescope in 2016. The image showed the galaxy had little to no signs of a central bulge or any prominent structures (typical of Magellanic-type spirals). However, the telescope could resolve many stars, as well as several turquoise-colored star forming regions.^[6]