The galaxy presents as an elliptical-like morphology with a smooth, centralized light distribution. The shape is neither perfectly round nor elongated, appearing as an intermediary form. Some form of interaction with another galaxy, or possibly a past interaction event, may be occurring; although no clear signs of a major disturbance or ongoing merger are visible, there are hints of a minor disturbance. The estimated stellar mass is substantial. The moderate levels of inferred star formation suggest that some star formation activity is ongoing within the galaxy. The galaxy appears bluish-white in color, indicating that the stars are relatively hot and young.
