The galaxy presents as a spiral type, exhibiting a disk-like morphology. Spiral arms are visible, appearing loosely wound. A central bulge is present, though not particularly dominant in size. The disk appears to be oriented at an angle relative to our line of sight, but is not edge-on. There is no clear visual indication of a strong bar feature within the galaxy. The color suggests an intermediate age stellar population, perhaps with ongoing or recent star formation. Evidence of interaction or merging is not immediately apparent, though subtle disturbances cannot be ruled out.
