The galaxy presents as a structured object with notable features indicative of potential interaction or merging activity. It displays an elongated shape with a dominant yellowish-orange hue, suggesting an older stellar population. A central, brighter region is visible, potentially indicating a galactic bulge or core. Extending from this central region are diffuse, less prominent features that create a bridge-like structure. A blueish-white region is at the far end of the galaxy. Morphological analysis suggests possible disturbances or tidal features that indicate the system is interacting with another galaxy. The red shift is ~0.29, so the galaxy is far enough that it is harder to determine whether this is a merger or not. 
