The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated light profile, indicative of a significant bulge component. The color is predominantly yellow-orange, suggesting an older stellar population. The galaxy displays a slight elongation, but generally appears quite symmetrical. No prominent spiral arms or significant dust lanes are discernible within the available image resolution. There is a hint of a more diffuse outer halo, but it lacks distinct features. There is no apparent active galactic nucleus or star formation. The galaxy appears relatively isolated, without any evident signs of recent major merger activity or tidal disturbances.
