The galaxy presents with a primarily smooth morphology, exhibiting a bright, concentrated central region. There is evidence of some irregular features or disturbances in the surrounding area, possibly indicating ongoing or past interaction with another galaxy. The galaxy's color profile suggests an older stellar population in the central bulge, with bluer colors radiating outwards, hinting at younger star formation in the outer regions. The overall shape appears relatively symmetric, though subtle asymmetries cannot be ruled out. A small part of the galaxy looks like it is undergoing a merger event.
