The galaxy presents a generally elliptical morphology. The light distribution appears relatively smooth with a centrally concentrated, bright core. There is a clear colour gradient, shifting from a yellowish-white hue at the core to a bluer tone in the outer regions of the galaxy. This colour variation suggests a radial change in stellar populations, with older, redder stars dominating the core and younger, bluer stars present in the surrounding regions. There are hints of subtle structural features, possibly suggestive of a disk component, but the overall appearance is dominated by its smooth, elliptical nature. The galaxy does not show obvious signs of a major merger or strong tidal disturbances, but subtle asymmetry could point to past minor interactions or ongoing accretion. The extent of the galaxy appears significant, implying a considerable physical size.
