This galaxy appears to be undergoing a major merging event. Two distinct components are visible, one appearing more rounded and smoother, while the other shows a less uniform structure, possibly indicative of tidal disruptions. There is a presence of some redder hues, particularly noticeable in the area with less uniform structure, suggesting an older stellar population or dust obscuration. Overall, the system displays a relatively diffuse appearance, without well-defined spiral arms or a prominent central bulge. The overall color suggests a galaxy with a moderately evolved stellar population, and a low star formation rate.
