This galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that gradually diffuses outwards. The color profile suggests an older stellar population, primarily composed of evolved stars, with a yellowish to reddish hue dominating the core. There's little evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or tidal interactions. Its overall form indicates a system transitioning toward a more quiescent state, with limited ongoing star formation. The object is moderately luminous and relatively massive, suggesting it is a mature galaxy within its population.
