This galaxy appears to be undergoing a merging event. One component is a relatively smooth elliptical or lenticular galaxy exhibiting a somewhat rounded morphology. It exhibits a yellow-white hue, suggesting an older stellar population. The second component exhibits a disk-like structure, seen nearly edge-on. This feature displays a distinct reddish-orange color, suggesting a significant dust content or a population of older stars. There is evidence of some disturbance in both components of the galaxy, which is most likely caused by tidal interactions between the merging galaxies. There appears to be a relatively low rate of recent star formation. The galaxy's overall size appears to be of moderate extent.
