The galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a bright, concentrated central region, suggesting a high stellar density in the core. The light profile appears to fade gradually from the center outwards, with no clear distinct features such as spiral arms or a prominent disk. There's a subtle color gradient observed. The central region shows hints of bluish-white hues, possibly indicating the presence of some younger, hotter stars or ongoing star formation, though this activity appears subdued. The outer regions seem redder, indicative of an older stellar population. Overall, the galaxy presents a settled, undisturbed morphology, likely an evolved system with a significant fraction of older stars and minimal ongoing merger activity.
