The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The central region exhibits a bright, yellowish-orange hue, suggesting a population dominated by older stars. Moving outwards from the center, the galaxy shows a gradual decrease in surface brightness. There is subtle bluer light in the outskirts of the galaxy, likely indicating younger star formation. The galaxy appears relatively undisturbed, with no obvious signs of a major merger or tidal interactions. It seems to be an isolated galaxy with a well-defined structure, though a minor asymmetry can be seen when looking at the object overall, indicating perhaps a minor interaction with another nearby object.
