The galaxy presents as a disturbed system, possibly undergoing a merger or significant tidal interaction. Two distinct luminous regions are visible. The dominant and more elongated structure appears to be a disk galaxy seen at a moderate inclination. Within this disk component, there appears to be a central bulge, but the bulge is not very pronounced. Patches of blue light are also visible in the disk.

The second region, less extended and more spherical, appears to be an irregular or dwarf galaxy undergoing an interaction with the disk galaxy. Some diffuse blue light is noted here as well, which may be an indication of active star formation in the interacting region. Evidence of tidal streams or bridges is not obvious in this image, but the overall morphology suggests an ongoing interaction or recent merger.
