The galaxy presents as a moderately luminous object with a red-shifted spectrum. Morphologically, the galaxy appears to be undergoing a significant interaction or merger. The main body of the galaxy exhibits a smooth, elliptical profile, with a concentrated central bulge. A smaller, distinct component is observed in close proximity, suggesting either a minor merger event or tidal disturbance. The overall color is relatively uniform, indicating an older stellar population with moderate star formation activity. The mass of the galaxy is substantial, suggesting a relatively evolved system.
