This galaxy presents an elliptical morphology, appearing somewhat smooth with hints of a flattened disk-like structure. Its color gradient indicates a bluer central region, possibly suggesting the presence of a younger stellar population or ongoing star formation activity towards the core. The outer regions appear redder, potentially signifying an older stellar population. There is also a possibility of a minor interaction or disturbance given the slight asymmetry in its shape. It doesn't appear to be undergoing a major merger, but close inspection of higher-resolution imagery may reveal finer tidal features. Overall, it seems to be an intermediate mass galaxy at a moderate redshift, showing signs of recent, or ongoing star formation.
