The galaxy presents a morphology indicative of a transition between a smooth elliptical form and a more complex, potentially disk-dominated structure. The central region appears relatively smooth and concentrated, while the outer regions exhibit subtle features hinting at spiral arms or tidal disturbances. There is evidence of ongoing star formation. The overall colour suggests a mix of stellar populations, with both older, redder stars and younger, bluer stars contributing to the galaxy's integrated light. There seems to be ongoing or recent merger events which have resulted in disturbances in the galaxy's disk.
