Messier 74

[7] The galaxy's low surface brightness makes it the most difficult Messier object for amateur astronomers to observe.

[13] The latter was bright as 10th magnitude when viewed from the surface of Earth, so visible from almost all modern telescopes in a good night sky.

[13] SN 2002ap was one of few Type Ic supernovae (which denotes hypernovae) recorded within 10 Mpc every century.

[3] Ben Sugerman found a "light echo" – a later reflection of the explosion – associated with SN 2003gd.

[20] Later analysis argued that it was consistent with known examples of giant LBV eruptions and SN 2008S-like objects.

Such an object is believed to form from lesser ("stellar") black holes within a star cluster.

[9] [8] This galaxy may be best viewed under low magnification; when highly magnified, the diffuse emission becomes more extended and appears too faint to be seen by many people.

[9] Additionally, M74 may be more easily seen when using averted vision when the eyes are fully dark adapted.

M74 observed by JWST
M74 as observed with the Spitzer Space Telescope as part of the Spitzer Infrared Nearby Galaxy Survey . The blue colors represent the 3.6 micrometre emission from stars. The green and red colors represent the 5.8 and 8.0 micrometre emission from polycyclic aromatic hydrocarbons and possibly dust.