The galaxy presents a generally smooth, elliptical morphology. It appears as a centrally concentrated spheroid with a gradual decrease in luminosity outwards from the core. The central region exhibits a bright, concentrated light, possibly indicative of a galactic nucleus. There is a subtle color gradient present, transitioning from a slightly redder hue in the core to a bluer tint in the outer regions. The galaxy shows no apparent spiral arm structure or significant dust lanes, suggesting it is not a spiral galaxy. There is a slight hint of a disk-like structure, though faint. There is no obvious evidence of tidal disturbances or ongoing mergers, however a minor interaction cannot be ruled out.
