The galaxy appears to be in a late stage merger. Two distinct components are visible. The first appears roughly spheroidal and has a yellowish-orange hue. The second component is more compact and has a blue color. This suggests a difference in stellar population between the two components, with the bluer component containing a greater proportion of younger, hotter stars. There are morphological disturbances visible, with asymmetry indicating tidal interactions between the two components. There is no discernable dust lane or spiral structure. Overall, it appears that these two galaxies are in the process of merging into a single object.