The galaxy presents as a generally smooth and rounded structure with a concentrated central bulge. The color profile suggests a population of older stars, with a yellowish-orange hue dominating the central region. There is a subtle gradient in color, transitioning to a slightly bluer, less intense outer halo, indicating the presence of some younger stars in the galactic periphery, though likely in lower concentrations. No prominent spiral arms or distinct features such as dust lanes are discernible. There is a slight elongation to the structure, but the morphology is primarily spheroidal. Overall the galaxy appears relatively undisturbed, showing no strong signs of ongoing merger activity or significant tidal distortions.
