This galaxy appears to be undergoing a significant interaction or merger. The primary body shows a disturbed morphology, with an extended, irregular shape rather than a clear spiral or elliptical form. There is a suggestion of tidal features or debris extending outwards. The color gradients across the galaxy are notable, with a central, yellowish-orange region possibly indicating an older stellar population, contrasted by bluer and greener areas that may signify regions of active star formation. A secondary, more compact, yellowish-orange component is visible and connected to the main galaxy, potentially representing a merging galaxy or a tidal dwarf galaxy. The overall structure points towards a dynamic system likely experiencing gravitational disruption and enhanced star formation activity.
