This galaxy presents as a centrally concentrated elliptical system. The core is luminous and exhibits a yellowish-white hue, potentially indicating an older stellar population. The galaxy appears relatively smooth in texture, with a minimal presence of distinct features like spiral arms or prominent dust lanes. The outer regions fade gradually, forming an elliptical halo that is nearly circular, showing a slight flattening. The overall color profile transitions from the warmer core to cooler, bluer tones in the outer reaches, suggesting the presence of younger stars at the periphery, although the star formation rate is low. The morphology is largely undisturbed, lacking clear signs of recent major mergers or tidal interactions.
