The galaxy presents a somewhat disturbed morphology. It is elongated, appearing disk-like but without a clear spiral arm structure. The central region displays a concentrated, brighter yellowish hue, possibly indicating an older stellar population or a more active galactic nucleus. Fainter, blue-green diffuse light extends outward, suggesting regions of more recent star formation, although these appear patchy and irregular. There is a hint of tidal features. Overall, the galaxy exhibits characteristics indicating a possible ongoing interaction or recent merger event.
