The galaxy presents an overall ellipsoidal morphology, appearing somewhat flattened. The central region is characterized by a bright, concentrated core. Surrounding this core is a diffuse, extended disk. Within this disk, there is evidence of some structural irregularities, though distinct spiral arms are not clearly visible. The color distribution suggests a fairly uniform stellar population across the galaxy. There is potentially some interaction or disturbance of this object due to the merging signature, which would likely result in the somewhat amorphous shape.