This galaxy appears to be of intermediate redshift and magnitude. It is neither extremely bright nor faint. The galaxy appears as a disturbed disk galaxy. There seems to be a central bulge or concentration of light, but the light is extended and not sharply defined. A flattened disk component is evident, but its structure is irregular with hints of dust lanes. The galaxy shows clear signs of interaction or disturbance; possibly a merger or tidal interaction. Patches of bluer light, presumably indicating recent star formation, are observed in the disk, although it could be a background object. Overall, the galaxy exhibits a distorted morphology, suggesting an ongoing dynamic process. 
