The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness moving outwards from the core. The galaxy's morphology is generally round, showing minimal signs of strong tidal interactions or major disturbances. There is a subtle suggestion of a disk or faint spiral arm structure, but this feature is not prominent. The central region appears bluish-white, potentially indicating the presence of a population of younger, hotter stars, while the outer regions tend towards red, indicating the older, cooler population of stars. The overall color suggests a mild level of ongoing star formation.
