The galaxy appears to be a spiral galaxy viewed at a slight angle, possibly with a weak central bulge. Some disk and spiral arm features are visible but indistinct. Blue hues suggest regions of ongoing star formation, although the overall star formation rate appears to be relatively low. Redder colors are observed within the central region. The system does not appear to be undergoing any major merger activity, though some minor tidal disturbances cannot be ruled out. The luminosity suggests a relatively massive galaxy. The relatively smooth appearance could indicate a more evolved system.
