The galaxy exhibits a smooth, elliptical morphology with a high degree of central concentration. The core region presents a bright, yellowish hue, indicating an older stellar population and a paucity of ongoing star formation in that area. A gradual decrease in surface brightness is observed moving outward from the core. The outer regions of the galaxy display a subtle bluer tint compared to the core, potentially suggesting a small amount of recent star formation, or a distribution of younger, bluer stars in the galaxy's halo. No distinct spiral arms or prominent dust lanes are visible. There is no evidence of a major ongoing merger, but there could be a faint minor disturbance. The galaxy presents a generally undisturbed, relaxed appearance.
