The galaxy presents as a system of multiple components, likely interacting. Two components appear yellowish with a smooth morphology, suggesting older stellar populations. The third component exhibits a bluer hue, indicative of ongoing or recent star formation. This component is less defined in shape. There is evidence of minor tidal disturbance in this galaxy system. The overall structure suggests a possible merger in progress, with the bluer component potentially a dwarf galaxy being accreted, or a region of heightened star formation triggered by gravitational interaction between these galaxies.
