The galaxy presents as a relatively smooth, elliptical structure. A bright, concentrated central bulge is visible, surrounded by a fainter, more diffuse halo. The overall color gradient suggests a higher concentration of older stars toward the center, with bluer colors indicating the presence of some younger stellar populations in the outer regions, though these regions are not particularly prominent. The galaxy displays a slight elongation, deviating from a perfect circular shape. There is no strong evidence of spiral arms or other distinct features typically associated with disk galaxies. The smooth texture and lack of prominent features suggests that this is a relatively undisturbed galaxy that is not currently undergoing a major merger event.
