The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light profile suggests it is a passively evolving system with an older stellar population as indicated by its yellow-red hue. There is a slight elongation and a hint of a disk but this is not a spiral galaxy. There is no indication of strong star formation regions, tidal tails, or recent merger events. Its overall morphology is consistent with an early-type galaxy in relative isolation.