The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution appears fairly uniform across the main body, with a gradual decrease in intensity from the core outwards. There is a subtle color gradient, transitioning from a yellowish-white core to a slightly redder outer halo. No distinct spiral arms or prominent dust lanes are readily apparent. Based on its morphology, the galaxy seems undisturbed, exhibiting no major signs of recent mergers or tidal interactions. There is evidence of ongoing, though possibly low, star formation.
