The galaxy presents an overall elliptical morphology, appearing somewhat compact. It exhibits a bright, concentrated central region, suggesting a prominent galactic nucleus. The core displays a bluish-white hue, potentially indicative of a population of younger, hotter stars. There is evidence of subtle features surrounding the core, possibly representing faint spiral arms or tidal disturbances. The galaxy displays slight asymmetry, particularly in the outer regions, hinting at potential gravitational interaction or recent merger activity. The observed color gradients suggest variations in stellar populations or dust distribution across the galaxy. A faint, reddish halo is present, extending beyond the main body, which could be attributed to an older stellar population or dust scattering.
