The galaxy presents an overall elliptical morphology, appearing somewhat elongated. A central, bright core dominates the structure, indicating a concentration of luminosity in the galactic nucleus. Fainter extensions emanate from this central region, displaying a diffuse halo. There is some evidence of asymmetrical features. A slight tidal disturbance or minor interaction may be indicated, but the overall structure maintains a relatively undisturbed elliptical form. Color gradients within the galaxy are subtle, with a tendency for the core to exhibit a slightly bluer hue compared to the more redshifted halo, possibly indicating populations of younger stars in the central regions. 
