The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile. The central region is bright, suggesting a high stellar density and potentially an active galactic nucleus. The isophotes appear relatively regular, indicating a relaxed, dynamically evolved system. No prominent spiral arms, bars, or dust lanes are visible. The overall color is slightly blue shifted toward the center of the galaxy. There is no clear tidal debris visible, which indicates that the galaxy is likely not undergoing a major merger.
