The galaxy presents as a single, relatively smooth structure with no distinct spiral arms or bar visible at this resolution. Its shape is predominantly round, exhibiting high degree of circular symmetry. The galaxy appears as a concentrated luminosity, with the light profile decreasing smoothly from the core outwards. There are no signs of major disturbances in its structure. The colour appears subtly reddish suggesting an older stellar population and a suppressed star formation rate. Its apparent size indicates it is likely a massive object at a significant distance, inferred from its redshift.
