The galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated, with a bright core that gradually diminishes outwards. There is no discernible spiral arm structure or significant dust lane obscuration. The galaxy is largely featureless, showing only a subtle change in color gradient from a whiter core to a bluer outer halo. There is no indication of recent or ongoing major merger events. The lack of distinct features indicates a potentially older stellar population with relatively low star formation activity.
