The galaxy appears to be a relatively smooth, elliptical galaxy at a significant redshift, suggesting a considerable distance. It exhibits a predominantly yellow/orange hue, which could indicate an older stellar population with a lower rate of ongoing star formation. The overall shape is elliptical, though it appears somewhat elongated and "in-between" roundness. No significant spiral arm structure or disk features are readily apparent, and the core is significantly brighter than the edges. There is no visually prominent indication of any major ongoing merger activity or tidal disturbances and is only minor.
