This galaxy exhibits a moderate redshift, indicating it is at a considerable distance. The overall morphology appears to be relatively smooth, although there may be some signs of disturbance or interaction. The galaxy appears elliptical or lenticular, and it has a notable elongated shape.

The color gradient suggests differential stellar populations and dust distribution. The central region displays a bluer hue, which could indicate a younger stellar population or ongoing star formation in that area. There is also evidence of ongoing merger activity and significant gravitational disturbance.
