The galaxy presents a generally smooth and elliptical morphology. There is a distinct, red-shifted central bulge. A less defined, greenish disk-like structure surrounds the bulge, suggesting possible ongoing, though subdued, star formation activity, particularly in the outer regions. The overall structure appears relatively undisturbed, without evidence of significant ongoing mergers or tidal interactions. The lack of strong blue coloration indicates a lower proportion of young, massive stars, pointing towards a more evolved stellar population. The galaxy appears to be moderately massive.
