The galaxy presents a somewhat elongated morphology, exhibiting a notable degree of disturbance. It is unlikely to be a spiral galaxy. There is no visual evidence of a prominent disk structure. The color appears to be generally blue-white, hinting at the presence of younger stellar populations, and there appears to be significant amounts of ongoing star formation. The light is more concentrated in the central region with a fuzzy halo, suggesting that the system is moderately massive. There may be interaction with another nearby galaxy or the aftermath of a recent merger event.
