Angular distance to the nearest companion:

magnitude:

questionable object (a star or a defect) near the galaxy

nearby faint galaxy

faint component

Component type:

Number of faint components:

Angular separation:

galaxies embedded in a common nebulous envelope

clear evidence of structure distortion

halo

unusual branched feature, e.g., a jet, streamer, or plume


tail

Distortion type:

blended galaxies

interaction at a distance

galaxies embedded in a common nebulous envelope

chain of galaxies

nest of galaxies

galactic nuclei in contact

galaxies in contact

galaxies connected by a spiral arm

galaxies connected by a bar

Interaction type:

suspected

evident

Interaction certainty:

Number of members observed to be interacting:

One of the fainter members of a ternary system.

Brightest member of a ternary system.

Another member of a binary system.

Member of a binary system.

One of the fainter members of a multiple system.

Brightest member of a multiple system.

 MCG

A companion galaxy is present.

Membership in a multiple system:

Nearby cluster number in the CGCG:

 janskys

5000 MHz:

2700 MHz:

1400 MHz:

780 MHz:

178 MHz:

Radio flux density observed at:

integrated B-V color:

integrated U-B color:

Color index:

Number of H II regions:

Total number of supernovae observed in this galaxy:

 km/sec

Rotational velocity:

Heliocentric radial velocity:

The spectrum contains emission lines.


Integral spectrum:

Number of galactic nuclei seen in contact:

Position angle:

edge on

one quarter

two quarters

three quarters

face on

Inclination of the principal plane to the line of sight:

image barely visible

black image

black image

black image

black image

completely black image

of the second outer region:

of the first outer region:

of the inner part:

Surface brightness:

across the minor axis of the entire galaxy:

across the major axis of the entire galaxy:

along the minor axis of the bright inner part:

along the major axis of the bright inner part:

Angular diameter:

Number of galaxies included in the combined magnitude:

The  magnitude given is that of two or more galaxies.