The galaxy presents as a moderately luminous, elliptical morphology. The central bulge exhibits a concentrated, yellowish hue, suggestive of an older stellar population. The surrounding halo is more diffuse with a faint bluish tint, potentially indicating a younger population of stars or ongoing star formation, albeit at a relatively low rate. The galaxy appears mostly undisturbed with no obvious signs of tidal interactions or recent mergers. The overall structure suggests a system that is transitioning to a more passive evolutionary stage.
