The galaxy presents a generally smooth, elliptical morphology. The central bulge exhibits a bright, concentrated luminosity, suggestive of a high stellar density. There is a subtle color gradient visible, transitioning from a slightly bluer hue at the outermost edges of the galaxy's halo to a yellower, redder tone towards the nucleus. This could indicate ongoing, albeit subdued, star formation in the outskirts, with older, redder stellar populations dominating the central region. There are minimal visual signs of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, without any obvious indications of recent or ongoing major merger events. Minor asymmetries or faint tidal features cannot be ruled out with this image resolution, but no prominent distortions are readily apparent. The overall shape is moderately elongated.
