This galaxy appears to be undergoing a significant interaction, possibly a merger. The system presents as two primary concentrations of light, suggesting two distinct galactic nuclei or dense stellar regions. The morphology is disturbed, with a general lack of defined spiral arms or a prominent disk. The light from the galaxy is yellowish-red, potentially indicating an older stellar population. There is no prominent dust lane visible. There is a faint suggestion of tidal features and disturbed morphology which is suggestive of an ongoing merger event.
