The galaxy presents a complex morphology suggestive of an ongoing or recent interaction or merger event. A dominant, relatively smooth component is visible, possibly representing the remnant core of a larger progenitor galaxy. A fainter, more diffuse structure is detected, which has evidence of tidal tails or distorted spiral arms extending from it. There may be a second galactic center in this area. These extensions are asymmetric, indicating gravitational disruption.

Dust lanes are visible within the galaxy, particularly in the central region and potentially in the tidal features. They are irregular in shape and distribution. Patches of star formation are visible as bright, blue knots throughout the galaxy, which are mostly in the tidal features. The overall color of the galaxy is somewhat blue, indicating the presence of a young stellar population, although some of the central region appears more yellow and/or red. The galaxy has a small, distinct core.
