The galaxy presents as a moderately bright, elongated elliptical or lenticular system. The core exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population with reduced ongoing star formation. The galaxy lacks prominent spiral arm structures or distinct dust lanes. The overall color profile indicates a relatively passive galaxy. The outskirts of the galaxy appear somewhat diffuse, fading gradually into the background sky, with a subtle gradient in color towards redder wavelengths. There's a very slight indication of a tidal feature or minor disturbance on one side, suggesting a potential past interaction with another galaxy, though it is very minimal. The galaxy's morphology is predominantly smooth, with no signs of intense star-forming regions visible in this band.
