
NGC 4725 · galaxy
NGC 4725
NGC 4725 is an intermediate barred spiral galaxy with a prominent ring structure, located in the northern constellation of Coma Berenices near the north galactic pole.
Image: en:NASA , en:WikiSky. Public domain, via Wikimedia Commons.
Identity & coordinates
Identification
- Primary designation
- NGC 4725
- All designations
- NGC 4725
- Object type
- Galaxy
- Constellation
- Coma Berenices
- Best viewing
- Spring
Coordinates & physical
- Right ascension (J2000)
- 12h 50m 26s
- Declination (J2000)
- +25° 30' 02"
- Apparent magnitude (V)
- —
- Distance
- —
- Redshift (z)
- 0.004033
Visibility tonight
The science
NGC 4725 is an intermediate barred spiral galaxy with a prominent ring structure, located in the northern constellation of Coma Berenices near the north galactic pole. It was discovered by German-born British astronomer William Herschel on April 6, 1785. The galaxy lies at a distance of approximately 40 megalight-years from the Milky Way. NGC 4725 is the brightest member of the Coma I Group of the Coma-Sculptor Cloud, although it is relatively isolated from the other members of this group. This galaxy is strongly disturbed and is interacting with neighboring spiral galaxy NGC 4747, with its spiral arms showing indications of warping. The pair have an angular separation of 24′, which corresponds to a projected linear separation of 370 kly. A tidal plume extends from NGC 4747 toward NGC 4725.
Summary adapted from Wikipedia · CC-BY-SA-4.0
References
- SIMBAD Not resolved
- NED Fetched May 8, 2026 View in NED ↗
- Wikipedia Fetched May 8, 2026 Read full article ↗
Wikipedia title resolved via id — the catalog designation was a Wikipedia article title directly.
1 merge conflict resolved
- coordinates: SIMBAD missing → NED used



