The galaxy exhibits an overall elliptical morphology with a bright, concentrated central region, potentially indicative of a significant galactic nucleus. The galaxy displays color gradients, shifting from a predominantly bluish hue at the core to greenish-yellow tones in the outer regions. This suggests variations in stellar populations or dust content across the galaxy. There is a suggestion of a slight asymmetry or disturbance in the galactic structure. Overall, this galaxy is likely experiencing some level of interaction or disruption in its galactic morphology.
