The galaxy presents a smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decrease in surface brightness towards the outer regions. The color profile is relatively uniform across the galaxy, with a slightly bluer hue in the central region which might suggest a weak active galactic nucleus or recent star formation. It exhibits a moderately elongated shape, and there are no distinct features such as spiral arms or a prominent disk component visible, although the minor disturbances may not be noticeable at this resolution. No signs of major ongoing mergers or tidal interactions are apparent.
