The galaxy presents as a relatively smooth, elliptical-like structure with a slight elongation. The central region exhibits a pronounced brightness, suggesting a high concentration of stars and potentially an active galactic nucleus. There is a noticeable color gradient from the center outwards; The central portion is a blue hue that fades into redder colors further away from the center. The smooth texture implies a lack of significant spiral arms or prominent dust lanes. There is no obvious ongoing merger or major disturbance.