The galaxy presents as a centrally concentrated, elliptical morphology. The light profile is smooth, exhibiting a gradual decrease in surface brightness from the core outwards. There is a distinct absence of spiral arm structures or prominent dust lanes. The color is primarily yellowish-orange, suggesting an older stellar population and a reduced rate of on-going star formation. No signs of tidal disturbances or recent merger activity are apparent, and the galaxy appears relatively undisturbed.
