The galaxy presents as a luminous, elliptical morphology, with a smooth, concentrated light profile. The central region exhibits a bright yellowish hue, suggesting an older stellar population or significant dust obscuration. There appears to be a subtle color gradient, transitioning to a slightly bluer tint in the outer regions, potentially indicative of younger stars or ongoing star formation, though at a low rate. No distinct spiral arms or bar structures are discernible. The overall appearance is of a relatively undisturbed system, without any major signs of tidal interactions or recent merger events.
