Messier 89

Current observations allow the possibility that M89 may be nearly perfectly spherical. Distinct flattening as ellipsoids is found in all easily measurable comparators up to a few times of its distance. The alternative explanation is that it is an ellipsoid oriented so that it appears spherical to an observer on Earth.

The galaxy features a surrounding structure of gas and dust, extending up to 150,000 light-years and jets of heated particles up to two-thirds of that. This indicates that it may have once been an active quasar or radio galaxy. M89 has an extensive and complex system of surrounding shells and plumes, indicating that it has seen one or several notable mergers.

Chandra studies in the wavelength of the X-Rays show two ring-like structures of hot gas in M89's nucleus, suggesting an outburst there 1 to 2 million years ago as well as ram-pressure stripping acting on the galaxy as it moves through Virgo's intracluster medium. The supermassive black hole at the core has a mass of (4.8±0.8)×10⁸ M_☉.

M89 also has a large array of globular clusters. A 2006 survey estimates that there are 2,000 ± 700 of these within 25′. This compares to 150 to 200 of these thought (among which many proven) to surround the Milky Way.