The galaxy presents a complex morphological structure. It appears to be a faint, extended object with signs of significant disturbance. There's no clearly defined nucleus, but rather a diffuse central concentration. It appears the galaxy is undergoing a minor merger event, which is indicated by its irregular shape and presence of faint tidal features or debris. The redder regions are indicative of older stellar populations or dust obscuration. Overall, this object exhibits characteristics consistent with a galaxy experiencing gravitational interactions or recent merger activity. Further investigation is required to confirm the exact nature and evolutionary stage of this galaxy.
