The galaxy presents a morphology that leans towards smooth and elliptical. The overall color profile suggests an older stellar population, with a dominant reddish-orange hue. There is a possible disk structure, but it's very faint and tightly wound if it exists at all. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. The galaxy is relatively compact, with a well-defined central bulge. The presence of subtle green hues could indicate some residual star formation, but likely at a suppressed rate.
