The galaxy presents as an elliptical morphology, appearing predominantly smooth and spheroidal in shape. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. A gradual decrease in surface brightness extends outwards from the core, with the outer regions appearing fainter and more diffuse. Subtle color gradients are discernible, with the central region displaying a slightly yellower hue, potentially indicating an older stellar population. The overall structure appears undisturbed, showing no strong evidence of recent mergers or tidal interactions, implying a gravitationally relaxed system. The lack of distinct features, such as spiral arms or dust lanes, further supports its classification as an elliptical galaxy.
