The galaxy presents as a relatively smooth, concentrated object, exhibiting characteristics suggestive of an early-type morphology, potentially an elliptical or lenticular galaxy. The central region displays a high surface brightness, indicated by a prominent, yellowish-orange hue. Moving outwards from the core, the light gradually diminishes, transitioning to a bluer color. Some subtle features or disturbances can be detected in the disk, potentially indicating some past merger activity. The galaxy appears to have a moderate redshift, suggesting a considerable distance. It is estimated to be a massive galaxy. Star formation activity is estimated to be low.
