The galaxy presents an overall smooth appearance, with a dominant central bulge. There is some indication of disk-like features, but they are not strongly defined. The galaxy appears to be in a late stage merger or shows signs of significant tidal disturbances, potentially with another galaxy that might be the source of the disturbances. It has intermediate roundness, exhibiting a shape that is neither perfectly circular nor highly elongated. The object has a moderate redshift, indicating that it is at a significant cosmological distance. It exhibits strong luminosity across the observed bands, suggesting ongoing star formation within the galaxy. It also seems like the central areas of this galaxy are older than the outer regions.
