The galaxy presents as a relatively small, faint object with a redshift indicating a significant distance. The light distribution suggests a galaxy undergoing some form of interaction or disturbance. A significant portion of the light appears to be concentrated in a somewhat smooth but elongated central region, indicative of either an elliptical galaxy or the bulge of a spiral.

One side of the galaxy shows a more diffuse and irregular structure, possibly indicative of a tidal tail or a disrupted arm. There is a hint of bluer colors in this extended region, possibly indicating ongoing star formation. The central region exhibits a slightly redder hue. The overall morphology suggests a system with a mass estimate in the lower end, but may be in the process of acquiring more material. There is no apparent active galactic nuclei.
