The galaxy appears to be a relatively smooth, elongated structure. Its morphology suggests characteristics intermediate between a purely elliptical galaxy and a disk galaxy, possibly of an intermediate type. There is a bright central region. The color gradient shifts from bluer hues in what appear to be less concentrated areas to redder or yellower tones toward the center. The image suggests that there is very little to no major merger activity present in the recent history of the galaxy. The galaxy's morphology indicates a low rate of ongoing star formation. The system does not appear to be undergoing major disturbances or tidal interactions.
