The galaxy exhibits a morphology that suggests an ongoing or recent interaction or merger. A primary component presents with a distorted disk structure, possibly indicative of tidal forces. Bright, concentrated regions are visible within this primary component, one is a bright yellow core, with a secondary bright but less concentrated blueish region to its side. These regions may represent the core or areas of intense star formation activity within the disrupted galaxy. A secondary, distinct component is also visible. This component is much smaller and lacks clearly defined structure. There are suggestions of faint tidal tails or debris extending from the interacting system, further supporting the hypothesis of gravitational interaction. Overall, the galaxy displays characteristics of a dynamically active system undergoing significant morphological transformation.
