The galaxy presents as a relatively smooth, elliptical form, appearing somewhat elongated. A bright central bulge is evident, indicating a concentration of stellar mass and potentially a supermassive black hole at the core. The color profile shifts subtly from a warmer, yellow-orange hue in the central region to a slightly cooler tone in the outer regions. The lack of distinct spiral arms or prominent dust lanes suggests a more evolved system with a low rate of ongoing star formation. There's a very slight indication of minor disturbance, though overall the system appears stable and relatively unperturbed. Its overall structure is consistent with an elliptical galaxy, potentially of considerable mass, observed at a significant distance.
