The galaxy presents as a largely featureless elliptical or lenticular galaxy with a bright central bulge. The galaxy exhibits a smooth, diffuse light profile indicative of an older stellar population. The core displays a yellowish hue, suggesting a concentration of evolved stars. The galaxy appears generally round, with no obvious signs of significant tidal disturbances or ongoing major mergers. There may be faint hints of a disk-like structure subtly embedded within the galaxy. The halo region surrounding the bulge shows a slightly bluer tinge, which could indicate pockets of younger stars or recent, low-level star formation activity. Overall, it presents as a relaxed, relatively evolved system.
