This galaxy presents as a centrally concentrated object, roughly elliptical in overall shape. There is an indication of a disk, or at least a flattened structure. The color is predominantly bluish-white in the central region, suggesting a population of relatively young, hot stars. There is also an indication of some lower frequency redder light on the outer edges of the galaxy, indicating a population of older stars. The morphology appears somewhat disturbed, as there may be an ongoing merger with another smaller galaxy or another type of galaxy interaction. There is likely a smooth component to this galaxy in addition to potential disturbances.
