The galaxy presents an elliptical morphology, with a smooth, centralized bulge. The light distribution suggests a relatively uniform stellar population throughout the galaxy. The disk appears highly inclined, as evidenced by its elongated shape. The galaxy's light profile appears to be largely devoid of significant spiral arm structures or distinct star-forming regions. The color gradient indicates bluer hues toward the outer regions of the disk, with a redder central bulge. There is no evidence of a major ongoing merger, although some minor disturbances cannot be ruled out. The galaxy appears to be a relatively isolated system.
