The galaxy appears to be an elliptical galaxy, characterized by a smooth, relatively featureless light distribution. Its morphology is mostly round, leaning slightly in between elliptical and completely circular. There is a subtle, elongated structure present. The color index suggests it's composed primarily of older stellar populations. No spiral arms or prominent dust lanes are discernible. There is no obvious evidence of an ongoing merger or major disturbance of this galaxy. However, there is a slight chance of a minor disturbance. The central bulge is prominent. The overall visual impression is of a fairly evolved, quiescent system.
