The galaxy exhibits a generally smooth morphology, with a dominant, rounded shape. There is some evidence of possible minor disturbances or interactions present in the system, suggesting a non-negligible rate of mergers. The galaxy's light profile appears concentrated, with a relatively high fraction of light contained within its central region.

Based on the estimated redshift, the galaxy is at a significant cosmological distance, and its absolute magnitude indicates that it is a luminous object. The inferred mass suggests a massive galaxy, with estimated star formation rates on the lower end, indicating potentially lower rates of star formation. The galaxy displays varying colors across different spectral bands.
