The galaxy presents as a complex system, potentially undergoing an interaction or merger. The central region exhibits a bright, concentrated core, appearing relatively smooth in texture. A distinct blue hue dominates this core, suggesting a population of hot, young stars or intense star formation activity. A less defined, yellowish component extends outwards from this core. This component has a more irregular shape, possibly indicating disrupted morphology due to gravitational interaction. There is indication of tidal features, or stellar streams, emanating from this galaxy. These could be the result of the ongoing dynamic processes within the galaxy. Further spectroscopic analysis is needed to fully characterize the stellar populations, kinematics, and the nature of any ongoing interaction.
