The galaxy presents a largely smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggesting a high stellar density in the central region. The light profile diffuses gradually outwards, transitioning from a yellowish hue in the core to a faint greenish-blue tinge in the outer regions. This color gradient might indicate variations in stellar populations, with older, redder stars concentrated centrally and younger, bluer stars in the outskirts, though the galaxy appears to be largely composed of older stars. The overall structure appears relatively undisturbed, showing no obvious signs of ongoing major mergers or tidal interactions. The galaxy appears to be fairly rounded in shape, though there is some slight indication of a disk. The star formation rate appears to be low.
