The observed galaxy appears to be undergoing a significant merger event. Multiple distinct luminous clumps are visible, with the overall structure exhibiting a disturbed morphology rather than a well-defined spiral or elliptical shape. The central region displays a concentration of light. The galaxy's color is generally yellowish, which suggests an older stellar population, but there are also bluer regions, particularly near the luminous clumps. Some features may indicate tidal tails or bridges, but further analysis is needed to confirm this. The system has an apparent deviation from a circular shape and looks somewhat elongated.
