The galaxy presents as a relatively smooth, elliptical-like structure, though slightly elongated. The central region exhibits a high degree of concentration and appears to be quite luminous, displaying a yellow-orange hue. Moving outward from the core, the color gradually fades, and the light diffuses into the surrounding space. There is a fainter, blue region that may be a satellite galaxy or region of active star formation. The overall morphology suggests a system that has largely ceased significant star formation, with a dominant older stellar population evident in the central bulge. There is no clear presence of a prominent disk component or spiral arms, and no signs of recent or ongoing major merger activity can be discerned. 
