The galaxy presents as a relatively smooth, elliptical-like object, exhibiting a concentrated central bulge. There is evidence of possible tidal features or minor disturbances in the overall structure. Based on its redshift, the galaxy is at a significant distance, explaining the limited resolution. The observed color gradient suggests a generally older stellar population with relatively low ongoing star formation. There is a suggestion of ongoing or past merger activity, indicated by disturbances to the morphology and possibly a faint, extended halo. The galaxy's light is concentrated towards the center, indicating a possible supermassive black hole at the core. Overall, the galaxy appears to be a massive elliptical at intermediate redshift, potentially undergoing minor evolutionary changes.
