The galaxy presents as a centrally concentrated, elliptical system. It exhibits a smooth, diffuse light profile indicative of an older stellar population. The core region appears more luminous and displays a yellow-orange hue, likely due to the dominance of evolved stars. There is little evidence of prominent spiral arms or significant dust lanes. Faint, irregular features are visible, and some minor disturbance in structure may be present. The overall shape is largely circular, with slight ellipticity. The surrounding halo appears relatively smooth and integrated with the central bulge. There is no clear ongoing merger activity, though some subtle signs of interaction might be interpreted. Star formation appears to be low.
