The galaxy presents as a centrally concentrated, elliptical form, with a relatively smooth overall appearance. The primary light emission appears to originate from a central bulge, exhibiting a white to slightly yellow hue. Extending outwards from this core is a diffuse halo of light, transitioning to a bluish tint particularly at the galaxy's outer edges. The overall structure appears to be generally undisturbed, exhibiting no obvious signs of major mergers or tidal distortions, but may show signs of a minor disturbance based on visual asymmetries. The light distribution suggests a relatively evolved stellar population throughout the galaxy, with potential evidence of ongoing, though possibly declining, star formation in the outer regions.
