The object appears to be a spiral galaxy exhibiting a moderate degree of disturbance. The galaxy's disk is not clearly defined and shows some evidence of tidal features, possibly indicating an ongoing or recent interaction with another galaxy. There are no obvious distinct arms; instead the galaxy seems to have a more flocculent, patchy spiral structure. There is no clear central bulge and instead the light is quite diffuse throughout. The light is slightly more blue than red, implying some star formation. The size is likely to be approximately 2 to 3 kpc. The system has some internal structure that might indicate minor merger activity.
