The galaxy presents a largely smooth and elliptical morphology. There is a concentrated central bulge region that appears yellowish-orange in color, suggesting an older stellar population dominating this area. Fainter, bluer light extends outward from the core, potentially indicating younger stars or some ongoing star formation in the outer regions of the galaxy. There is a subtle hint of a disk structure within the outer regions, however, it is not very distinct. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal tails. The overall shape suggests that the galaxy is close to spheroidal in shape, but not quite. The galaxy does appear round.
