This galaxy appears to be in the process of merging or interacting with another galaxy. Two distinct, luminous bodies are visible, suggesting either two separate galaxies closely interacting or a single galaxy with a highly disturbed morphology resulting from a recent merger.

The overall color of the galaxy is yellowish, indicating a relatively older stellar population and/or significant dust obscuration. This is consistent with a lower rate of star formation. There is no apparent spiral structure. The dominant morphology is smooth and round, indicating that the object is likely to be an elliptical galaxy.