The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright yellowish-white luminosity, suggesting a relatively high density of older stellar populations. Moving outward from the core, the light gradually diminishes, transitioning to a reddish hue in the outer regions of the galaxy. No distinct spiral arm structures or prominent dust lanes are observable. The overall shape is somewhat elongated but approaches round, without significant distortions or tidal features to indicate recent major merger activity. The structure appears largely undisturbed, maintaining a smooth, regular profile.
