The galaxy appears to be a relatively smooth, elliptical-like structure. Its overall color profile suggests an older stellar population, potentially indicative of a galaxy that has largely ceased active star formation. There is minimal evidence of spiral arms or a prominent disk, suggesting that it is a morphologically evolved system. The light is highly concentrated in its central region, implying a high degree of sphericity. There does not appear to be any significant tidal features, obvious dust lanes, or signs of recent interactions or mergers. Overall, the galaxy presents itself as a quiescent system with little apparent substructure.
