The galaxy presents a generally smooth, elliptical morphology with high degree of central concentration. The light distribution appears regular and centrally bright, fading gradually outwards. There is a clear color gradient, shifting from a yellowish-white in the core to a more reddish hue in the outer regions. No distinct spiral arms or prominent dust lanes are apparent. There are no signs of major ongoing mergers or significant tidal distortions. The galaxy is very round with no disturbances. Based on these characteristics, it would appear to be a fairly massive system with a relatively low star formation rate.
