The galaxy appears to be in a late stage merger. Two distinct galactic nuclei are observed within a common, distorted halo. One of the nuclei exhibits a yellowish hue, while the other has a bluer tint. Tidal features are faint, suggesting a relatively smooth structure despite the ongoing interaction. The overall morphology leans toward spheroidal, with only minor hints of a disk-like component. There is evidence of ongoing or recent star formation.
