The galaxy presents as a somewhat smooth, elongated structure. The central region displays a distinct orange hue, possibly indicative of an older stellar population. Proceeding outwards from the center the color fades to a fainter white color. There is a hint of asymmetry or minor disturbance in the outer structure, potentially suggesting an ongoing or past interaction with another galaxy. The galaxy's overall shape suggests a morphology somewhere between elliptical and disk-like, with a moderate degree of roundness. There appears to be no strong evidence of a major ongoing merger.
