The galaxy presents an intermediate disk-like morphology with a prominent bulge. The disk component exhibits notable structure, with indications of spiral arm segments. These arms appear somewhat flocculent, exhibiting patchy regions of star formation. The overall color suggests a moderate amount of ongoing star formation. The galaxy appears to be undergoing a major merger. There is a distinct disruption in the galaxy's morphology as well as the appearance of tidal tails, indicating gravitational interaction with another galactic object.
