The galaxy presents an overall elliptical morphology with a smooth light distribution. The central region exhibits a high concentration of older stellar populations, indicated by its yellowish-orange hue. Moving outwards from the core, a faint bluish halo is observed, suggesting the presence of younger, hotter stars and possibly ongoing star formation. The galaxy appears relatively undisturbed, with no prominent tidal features or asymmetries indicating recent major mergers. A slight elongation is noticeable, giving it a somewhat flattened, in-between roundness shape. There are indications of minor disturbances within the galaxy's structure.
