The galaxy presents a largely smooth morphology, exhibiting minimal discernible features such as spiral arms or a prominent disk. Its overall shape appears elliptical, with a high degree of roundness. Color gradients suggest a central concentration of older stellar populations, indicated by the yellowish hue at the core, gradually transitioning to a greenish tinge towards the outer regions. The lack of significant morphological disturbances points toward a state of relative quiescence, with no evident signs of recent major mergers or interactions. Overall, the galaxy appears as a relatively evolved system.
