The galaxy appears as a multi-component system, exhibiting a dominant central spheroid with a yellowish hue. This suggests an older stellar population. Adjacent to the primary spheroid is a distinct, smaller, bluish component. The color implies more recent star formation activity. There is a third component that is more diffuse and red in color, hinting at a potential tidal interaction or merger remnant. The roundness of the primary spheroid and the overall morphology of the system indicate a gravitationally bound structure that is potentially in the late stages of merging or experiencing a tidal interaction. The size of the galaxy is moderately compact. 
