This galaxy exhibits a moderate redshift, suggesting a considerable distance. Its morphology appears to be relatively smooth, however, it is not perfectly spherical and displays some features which indicate that it may have spiral or disk-like elements. There appears to be a notable central bulge with a high concentration of older stars, giving it a reddish-yellow hue. Fainter, bluer regions may be present, indicating younger stellar populations, although these are not well-defined. The light distribution across the galaxy is fairly concentrated, without extensive, diffuse outer regions. The overall shape appears moderately elliptical. It is of intermediate mass and exhibits a moderate amount of star formation. There is evidence suggesting it could be merging with another object.
