The galaxy presents a relatively smooth, elliptical morphology with a high degree of central concentration. The color distribution suggests a generally older stellar population, with a slight reddening towards the core. This is surrounded by a bluer and more diffuse halo. There is no obvious spiral structure or bar visible. There's no clear sign of any ongoing major merger activity. The galaxy is fairly symmetrical. Faint signs of minor disturbances or tidal features cannot be ruled out. The overall appearance suggests an early-type galaxy with a significant mass and a relatively low star formation rate.
