The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, centralized light distribution with minimal discernible spiral arm structure. There are no visible dust lanes. The primary color of the galaxy's light is a yellowish-orange hue, suggesting a population of older, redder stars dominates. The galaxy is somewhat elongated in shape. Faint bluish regions can be observed at the edge of the object. There are indications of disturbed morphology potentially resulting from a past or ongoing merging event. A faint blue-ish haze surrounds the bright central region, but the main galaxy does not appear to show any violent star formation. The mass of the galaxy is estimated to be large, and there appears to be moderate star formation taking place. The overall impression is of a relatively evolved galaxy in the distant universe.
