The galaxy presents as a merging system, or a galaxy undergoing a significant interaction. The morphology is disturbed, indicating a non-equilibrium state. Two distinct, bright components are visible. The color is generally yellowish, suggestive of a population of older stars. The round shape observed suggests that it is likely an elliptical galaxy type, but the interaction has greatly disturbed the roundness and shape. No obvious dust lanes or spiral arm structures are discernible. The presence of two prominent light concentrations indicates that there are distinct nuclei. The system appears relatively compact, with a concentration of luminosity in the central region.
