The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. The galaxy exhibits a radial color gradient, with a yellowish core that suggests a population of older stars. Moving outward from the core, the galaxy fades into a blueish halo. The intermediate roundedness indicates that the shape is neither perfectly circular nor highly elongated. The light distribution appears regular, without obvious signs of strong tidal features or recent major merger activity, though there is minor asymmetry visible. Overall, the galaxy gives the impression of being a relatively undisturbed system with ongoing, but mild star formation activity.
