The observed galaxy presents a complex morphology with evidence of multiple components. A prominent, nearly circular central region exhibits a bright, concentrated core that transitions to a fainter, diffuse halo. The central region displays a bluish hue, potentially indicative of younger stellar populations or active star formation. 

Above the center is a yellow glow that is either a strong arm of the galaxy or another galaxy interacting with it. The overall structure shows some irregularity, hinting at possible past interactions or ongoing merging events. There is no clear disk structure, but subtle features suggest minor disturbances. Some asymmetries exist in the outer regions, particularly in terms of color distribution.
