The galaxy presents as a centrally concentrated, smooth elliptical galaxy with a notable lack of discernible spiral arms or a prominent disk structure. It exhibits a generally round morphology. The light profile transitions from a bright, yellowish-white core to a diffuse, reddish-hued outer envelope. The color gradient suggests potential variations in stellar populations, with the core possibly dominated by older, evolved stars and the outer regions exhibiting a small amount of on-going star formation. There appear to be no signs of major ongoing merger activity or significant tidal disturbances.
