The galaxy presents an overall elliptical morphology, with a largely smooth light distribution. A subtle asymmetry in the outer regions suggests possible interaction or past merger events. There may be weak tidal features, but these are not clearly defined. The galaxy appears to be dominated by older stellar populations, based on the reddish-yellow hue of the central bulge. The low levels of blue light suggest relatively low levels of on-going star formation within the system. It appears relatively massive. The galaxy is more likely to be in the process of or has already quenched its star formation.
