The galaxy presents a somewhat flattened, elliptical morphology when viewed from our perspective. The central bulge appears luminous and concentrated, exhibiting a yellowish-orange hue, suggestive of an older stellar population. A faint, disk-like structure is present around the bulge. The disc is not sharply defined, and some degree of disturbance may be present. The apparent smoothness suggests a more evolved system, potentially in a transition phase. There is a subtle color gradient from the center towards the outskirts, with the outer regions appearing slightly bluer, which may point to ongoing, though subdued, star formation.
