The galaxy presents a complex morphology, appearing to be undergoing a significant interaction or merger with another galactic object. The main body of the galaxy displays a diffuse, somewhat amorphous structure, with a high degree of central concentration and relatively low degree of central asymmetry. There may be some degree of rotational flattening, but this is not particularly well-defined. There also appears to be an older stellar population within the galaxy, and indications of ongoing star formation. Star formation regions are not particularly prominent or tightly clustered. Overall, the galaxy displays a moderate amount of dust extinction.
