The galaxy appears to be a relatively bright object with a redshift indicating a significant distance. Its apparent size is small, yet estimated absolute magnitudes suggest considerable intrinsic luminosity. Morphologically, the galaxy presents a dominant smooth component, but also shows some features indicative of a possible disk or disturbance. It is neither perfectly round nor highly elongated, showing an intermediate shape. There may be a small chance of a minor disturbance present, but it is likely not undergoing a major merger at this time. The color profile suggests active star formation. The galaxy's mass is estimated to be relatively large. Star formation activity is present, but not at an extremely high rate.
