The galaxy appears as a relatively smooth, elongated structure. Its shape can be described as elliptical, with a high degree of roundness. The core region exhibits a concentrated brightness, fading towards the edges of the galaxy. The color profile appears to be consistent across the galaxy, with a yellowish-orange hue that suggests an older stellar population and a relatively low ongoing star formation rate. There are no visible spiral arms or significant dust lanes, which further supports its categorization as an elliptical galaxy. The galaxy does not show any obvious signs of a recent or ongoing merger event. The structure appears largely undisturbed.
