The galaxy presents as a relatively compact structure, with an overall elliptical morphology. The central region exhibits high luminosity, suggesting a concentration of older stars. A subtle color gradient is noticeable, transitioning from a warmer, yellowish hue in the core to slightly cooler tones toward the outer regions. Faint structural asymmetries hint at a possible ongoing or recent interaction or merger event. The system seems to be undergoing low rates of star formation. The galaxy appears fairly smooth and undisturbed, not exhibiting strong spiral arms or prominent dust lanes.
