The galaxy exhibits a central, bright, and concentrated core, which likely contains a supermassive black hole. Radiating outward is an elongated disk structure. The light distribution suggests an elliptical shape with a disturbed morphology. The disk shows some evidence of possible tidal interactions or minor disturbances. The bluer color suggests the presence of recent star formation activity in the outer disk, or that it is a blue compact dwarf galaxy. There is a faint and diffuse halo, which could indicate extended gas or stellar populations. Possible evidence of minor tidal interactions may be present.
