The galaxy exhibits a generally elliptical morphology. The light profile appears smooth and centrally concentrated, with a noticeable color gradient; the core region presents a yellow-red hue, gradually shifting towards blue-green as it extends outwards. There is no clear indication of spiral arm structures or prominent dust lanes. The overall structure suggests a relatively evolved system with little ongoing star formation in the central regions, although the outer parts show slightly younger stellar populations. There does not appear to be any active galactic nuclei, based on the lack of a bright and intensely radiating center. There are no visual signs of recent or ongoing major merger events. The galaxy is quite compact.