The galaxy presents a largely smooth, elliptical morphology. The light profile exhibits a strong central concentration, gradually decreasing in intensity outward. The core region appears bright and somewhat yellow, suggesting an older stellar population. The galaxy appears relatively undisturbed, with no obvious tidal features or signs of a major merger event. Faint, diffuse extensions are noted surrounding the central body. These extensions appear to have a more reddish color than the central region, which may indicate the existence of older populations of stars on the edges of the galaxy. The galaxy's shape is relatively round but with an intermediate shape, indicating that it's neither perfectly circular nor overly elongated. There are no distinctive features like prominent dust lanes or spiral arms. The overall structure indicates a system dominated by old stars, with little ongoing star formation activity.
