The galaxy appears as a single, relatively smooth object with a high degree of central concentration. The light distribution is highly symmetric, with a nearly circular isophotal shape. There is a color gradient across the galaxy, transitioning from a yellowish-white core to redder outer regions. There is no apparent spiral structure or disk component, nor signs of any ongoing major merger events, though some minor asymmetries may suggest past interactions. Given its high degree of smoothness and central concentration, along with the lack of visible star formation regions, it is likely an elliptical galaxy. The galaxy is relatively massive and has low star formation activity.
