The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. The color gradient suggests an older stellar population, with a redder core transitioning to slightly bluer outer regions. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits an elliptical or lenticular shape. There is a possibility of minor disturbances in the galaxy's structure suggesting interaction with another galaxy. Overall, the galaxy seems to be a relatively undisturbed system undergoing steady star formation.
