| NGC 4881 | |
| Type: | E0 |
| Dist Ly: | 94.62± |
| Appmag V: | 14.6 |
NGC 4881 is an elliptical galaxy in the northern constellation of Coma Berenices. It was discovered by the German astronomer Heinrich Louis d'Arrest on April 22, 1865. John L. E. Dreyer described it as "faint, small, a little extended, 9th magnitude star to southwest". This object is located at a distance of approximately 94.62Mpc from the Milky Way. It is a member of the Coma cluster of galaxies, positioned around to the north of the cluster's center with no nearby galactic neighbors.
The morphological class of this galaxy is E0, indicating it is an elliptical galaxy with a spherically symmetric form. It does not display any unusual or peculiar features. A total of 88 globular cluster candidates have been identified orbiting this galaxy, which yields an estimated total of . It has an unusually low frequency of globulars for a galaxy of this type.