The galaxy presents as a smooth, elliptical-like morphology. There is a concentrated central bulge region that transitions outwards to a diffuse halo. The galaxy exhibits a color gradient, appearing bluer towards its outer regions and more yellow-orange towards the central bulge, indicating the presence of older stellar populations. The galaxy shows a slight tilt relative to the observer's line of sight. There is no obvious evidence of spiral arm structure, and it lacks prominent dust lanes or signs of recent major merger events.
