The galaxy appears to be undergoing a significant interaction or merger. The overall morphology is disturbed, showing an irregular shape with a noticeable extended structure. There are no strong spiral arms visible.

The central region exhibits a brighter, concentrated luminosity, potentially indicating a dense galactic nucleus. The color gradient suggests varying stellar populations, with bluer hues mixed in with the yellow colors. This could be associated with on going star formation within the central region.

There are visible disruptions and extensions of the galactic material, possibly due to gravitational tidal forces. The galaxy's appearance is indicative of a relatively late-stage merger process.
