The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in intensity moving outward from the core. The galaxy exhibits a dominant yellow-orange hue in its central region, indicative of an older stellar population. A subtle, greenish-blue halo surrounds the core, suggesting the presence of some younger stars or ionized gas, albeit at a significantly lower rate than in typical star-forming galaxies. There are no clear signs of spiral arms or prominent dust lanes. The galaxy appears relatively isolated, with no obvious tidal features or nearby companions suggesting recent or ongoing mergers. The overall structure indicates that this is likely a well-evolved galaxy approaching a more quiescent stage of stellar evolution.
