The galaxy exhibits a centrally concentrated morphology, appearing relatively compact. The central region displays a bright, concentrated core. Surrounding this core, we observe a slightly extended, asymmetrical structure. Faint color gradients are present, transitioning from bluer hues in the inner regions to slightly redder tones in the outer regions of the disk. There appears to be some indication of disturbed morphology possibly caused by tidal interactions or merger activity. The image suggests the galaxy is undergoing some form of perturbation.
