The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. The central region exhibits a bright, concentrated core, suggestive of a significant stellar population. Proceeding outwards from the core, the intensity of light gradually decreases, forming a smooth halo. There is a slight elongation along one axis and the galaxy appears mostly undisturbed, without any indications of major mergers or tidal features. A yellowish tint to the core transitions to a greenish hue in the outer regions. The faint green light might indicate more active star formation in the outer regions compared to the yellow core. The overall structure is indicative of an evolved galaxy, with signs of older stellar populations.
