The galaxy appears to be a relatively smooth, elliptical galaxy with a centrally concentrated bulge. The light distribution is dominated by older stellar populations, as indicated by the reddish-yellow hue of the core region. There may be a weak disk component present, but it is not well-defined in this image. The galaxy exhibits a small amount of disturbance. There are no apparent tidal tails or strong signs of recent major mergers. The galaxy is approximately 6 kiloparsecs in radius. The overall morphology suggests that this is a passively evolving galaxy.
