A compact spiral galaxy in Canes Venatici with a small, bright centre. It has used up most of its gas: stars make up 96% of the mass it shines with, the largest share of any galaxy measured on this site.
Galaxy in Canes Venatici. Magnitude 8.2.
From Georgetown (6.8° N) it climbs to 56° above the northern horizon at its highest; from Lethem (3.4° N), to 52° above the northern horizon. It is highest at midnight on the night of 2 Apr, in the middle of its season. The page works out tonight's rise, highest point and set for both towns in Guyana time (UTC-4), and where the Moon is.
Apparent size from OpenNGC (Mattia Verga), CC-BY-SA-4.0.
Measured: What its visible mass is made of: stars and gas, not dark matter.
Each mass is given to a tenth of a dex, so each share is good to about a quarter of itself. Dark matter is not counted. Leroy et al. 2008, AJ 136, 2782, Table 4 (VizieR J/AJ/136/2782), NGC 4736: log stellar mass 10.3, atomic gas 8.7, molecular gas 8.6 (Suns). Shares do not depend on the distance the paper adopted.
Also in it, not measured:
How we know: Distance from its brightest red giants (the tip of the red giant branch): NED-D (NASA/IPAC Extragalactic Database, redshift-independent distances), median of 3 TRGB estimates: 4.66 Mpc, 4.20-4.66 Mpc; e.g. 2011ApJS..195...18R, 2009AJ....138..332J, 2003A&A...398..467K; retrieved 2026-10-21. True size: the apparent size times the distance (apparent size: OpenNGC (Mattia Verga, CC BY-SA 4.0), commit 4e2398a2).

More deep-sky objects: Sunflower Galaxy (M63) · Galaxy M106 · Whirlpool Galaxy (M51) · M109 (Galaxy) · Needle Galaxy (NGC 4565) · Pinwheel Galaxy (M101)