The galaxy appears as a relatively smooth, centrally concentrated elliptical galaxy. It exhibits a yellow-orange hue, suggesting an older stellar population with a lower rate of ongoing star formation. The galaxy shows a high degree of radial symmetry. There's no apparent spiral arm structure or significant dust lane obscuration visible in this image. It is a spheroidal galaxy, that does not show major disturbances in its galactic structure. It is estimated to have a large mass that would be in the range of a large galaxy.
