The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a distinct yellow-orange hue across its entirety, suggesting a likely older stellar population with a reduced presence of young, massive blue stars. The morphology appears predominantly elliptical, with a high degree of roundness. No prominent spiral arm structures or significant dust lanes are discernible. There is no indication of active galactic nucleus activity or a recent major merger event. The light profile fades gradually from the core outwards, with no sharp edges. The overall structure indicates that this is a relatively massive galaxy with suppressed star formation. 
