Kammala wannan magana: NGC 4395 an zana shi kuma an rarraba shi a matsayin "ƙuƙwalwar ƙuƙwalwa" a cikin takarda ta 1920 ta masanin astronomer Francis G. Pease. Yanzu, an san shi a matsayin galaxy daban daga Milky Way (duba
Babban muhawara). Tare da wasu taurari da ke kusa, taurari da aka ƙayyade a cikin NGC 4395 an yi amfani da su don auna yawan fadada sararin samaniya ta Allan Sandage da Gustav Andreas Tammann a cikin takardun su na 1974. Kwanan nan, an gano NGC 4395 don ƙunsar ƙananan ƙarancin haske mai aiki na galactic. Tun daga wannan lokacin, zuciyarta ta kasance batun wasu takardun ilimi da kuma ƙoƙarin auna yawan ramin baƙar fata na tsakiya.