The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution appears symmetrical with a gradual decrease in intensity from the core outwards. Faint color variations are discernible, hinting at underlying stellar populations. The core exhibits a yellowish hue, potentially indicating older stars, while the outer regions show a slightly bluer tint, suggestive of younger stars, or a population with a higher metallicity. No distinct spiral arms or dust lanes are apparent. Overall, the galaxy appears undisturbed, with no visual signs of major mergers or tidal interactions.
