The galaxy presents as an apparent merger of two distinct luminous regions. One region exhibits a more elliptical morphology, with a reddish-orange hue, suggesting an older stellar population or significant dust obscuration. The second region is less defined, displays a more greenish-blue color, and exhibits a more diffuse quality that may imply ongoing star formation. There seems to be a connecting bridge of material in the region between the two merging galaxies. The overall shape is somewhat amorphous, lacking a clearly defined spiral or elliptical structure, which supports the interacting system hypothesis. Faint outer regions surround the object, but are not distinctly defined.
