The galaxy appears to be undergoing an interaction, or at least a close passing, with another galaxy. One galaxy shows signs of a disk-like structure, with a slight bulge and a generally elongated shape that suggests it is not viewed perfectly face-on. This galaxy displays a yellowish hue, potentially indicating an older stellar population and reduced star formation.

The other galaxy exhibits a more amorphous and rounded shape, and has a bluer color, possibly due to the presence of younger, hotter stars. There is a suggestion of tidal disturbances. The shape of the brighter galaxy is distorted.
