This galaxy exhibits an irregular morphology, suggesting a possible ongoing or recent merger event. The central region displays a bright, concentrated core, surrounded by a less defined, diffuse halo of light. There is evidence of tidal features, possibly tails or streams of stars, extending outwards from the main body of the galaxy. These features are faint and stretched, indicating gravitational interactions with another galactic body. There also appears to be a potential disruption in the galaxy’s structure that could indicate it is undergoing a merger or some other form of galactic disturbance. Overall, the galaxy presents a disturbed appearance, indicative of ongoing gravitational interactions or a recent merger.
