The galaxy appears as a moderately bright, elliptical-shaped object. The galaxy's light profile is relatively smooth and concentrated toward the center, suggesting an older stellar population dominates. There is a slight elongation, but it is mostly rounded in shape. A subtle color gradient appears, hinting at possible variations in stellar population or dust content across the galaxy. There is some evidence of a minor disturbance or interaction, possibly with a smaller companion, or it could be a result of a previous merger event that is still visible in the galaxy's structure. It shows a relatively low ongoing star formation rate.
