The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated core is clearly visible, suggesting a substantial central mass concentration, possibly a supermassive black hole. The color profile is indicative of an evolved stellar population. The core appears yellowish-white, transitioning to a more reddish hue in the outer regions of the galaxy. The smooth light distribution supports a classification as an elliptical galaxy, lacking significant spiral arm structures or dust lanes. The galaxy exhibits a high degree of rotational symmetry with a round appearance. There is no obvious evidence of ongoing or recent major merger activity or tidal distortions. Any signs of minor disturbances are weak at best. Based on the colors and lack of distinct features, I would say star formation is low in this galaxy. The object has a spatial extent of approximately 5 kpc.
