The galaxy presents a largely smooth, elliptical morphology. There is an observed color gradient with the central region exhibiting a yellowish hue, possibly indicating a population of older stars. The outer regions display a bluer coloration. There's a slight deviation from perfect circularity, leaning towards an intermediate shape between round and elongated. No major disturbances or merger features are clearly discernible, although a minor asymmetry in the galaxy's shape can be seen. The galaxy is relatively compact. Overall, the galaxy appears to be a passively evolving system, with signs of a gradual decline in its star formation rate.
