This galaxy presents a generally smooth and rounded morphology. The central region exhibits a bright, concentrated core, suggesting a significant concentration of stars and possibly a supermassive black hole. The light profile appears to fade gradually from the core outwards. The galaxy's overall color is slightly on the bluer side, with some subtle variations in color across the body of the galaxy. There appears to be a minor visual disturbance, but overall the galaxy appears relatively undisturbed. Based on its morphology, it would be characterized as an elliptical galaxy. The galaxy exhibits an estimated radius of approximately 3.5 kpc. Its estimated mass suggests a substantial stellar population. The presence of some blue light suggests ongoing star formation, even though its rate may be relatively low.
