The galaxy exhibits a complex structure, potentially indicative of interactions or disturbances. The central region presents a bright, somewhat amorphous morphology with clumpy features. Surrounding this core, a fainter, more diffuse halo extends outwards. The overall shape is irregular, deviating significantly from a smooth elliptical or spiral form. There are hints of tidal features, perhaps subtle extensions or distortions in the outer regions, suggesting past or ongoing gravitational interactions. The color distribution reveals gradients, with bluer hues concentrated towards the center and redder tones in the outer halo. The galaxy displays multiple distinct light concentrations, which may indicate active star-forming regions or unresolved substructures. The image data quality limits precise morphological classification, but the overall appearance supports the hypothesis that this galaxy is dynamically active. 
