The galaxy presents as a diffuse object with a generally elliptical morphology. The central region exhibits a higher surface brightness, appearing as a concentrated core. Fainter extensions are visible, hinting at tidal features or distortions, possibly indicating past or ongoing interactions. The galaxy displays a color gradient, with the core appearing more yellow-reddish, suggesting an older stellar population, while the outer regions show bluer tones. The overall structure implies a potentially disturbed system, deviating from a typical, well-defined elliptical or spiral shape.