The galaxy presents as a smooth, centrally concentrated object. Its shape is elliptical, exhibiting a notable elongation. The color profile suggests an older stellar population, with a yellowish hue dominating the central bulge. The outer regions appear slightly bluer, hinting at some ongoing, albeit limited, star formation. There are no clear signs of spiral arms or significant dust lanes. The overall morphology points to a relatively evolved galaxy, likely of considerable mass, that has largely completed its major star formation phase. There are no obvious signs of tidal disruption or ongoing merger activity. It presents as a largely undisturbed system.
