The galaxy displays a disturbed morphology indicative of an ongoing interaction or merger. The primary galactic body appears distorted, with an irregular shape lacking a well-defined spiral structure. It exhibits a bright, concentrated central region, possibly a bulge or a region of intense star formation activity triggered by the interaction. Extending outwards from the main body is a distinct tidal tail composed of stellar material, dust, and gas. This tail stretches away from the galaxy. The color suggests a mix of stellar populations, with bluer regions potentially indicating younger, hotter stars formed during the interaction, and redder regions possibly composed of older stars or dust. No significant dust lanes are clearly visible within the main galactic body, though faint, diffused patches suggest the presence of dust clouds. There are hints of spiral arms or disk features being disrupted and pulled apart by the gravitational forces involved in the interaction.
