The galaxy presents an overall elliptical morphology, appearing largely smooth and featureless. The core exhibits a bright, concentrated luminosity, suggesting a high stellar density or a possible active galactic nucleus. The light distribution diminishes gradually outwards from the center, transitioning from a yellow-orange hue towards a slightly bluer outer region. The shape appears generally rounded, with no obvious signs of significant tidal distortions or ongoing mergers. There is a subtle hint of a disk-like structure, though the dominant characteristic is that of a spheroidal galaxy.
