The galaxy appears to be a spiral galaxy, possibly undergoing a merger or significant interaction with another galaxy. One section of the galaxy is a bright, somewhat diffuse, yellow-white elliptical form. Adjacent to this is a more clearly defined, disk-shaped component oriented at an angle. This disk exhibits subtle hints of spiral structure, though the arms are not sharply defined. The colour is generally bluer in the disk, suggesting the presence of younger, hotter stars compared to the elliptical section.

There is evidence of tidal disturbances or faint plumes extending from both components. There is no apparent central bulge. The system's overall morphology suggests a relatively low rate of star formation.
