The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. The core region exhibits a yellowish-orange hue, potentially indicative of an older stellar population. A faint, greenish halo surrounds the central bulge, possibly due to the presence of younger, bluer stars or ionized gas. There is a subtle hint of asymmetry or disturbance in the outer regions, though no major merger events are apparent. The overall morphology suggests an elliptical or lenticular galaxy, with limited evidence of spiral arms or significant disk structure.
