The galaxy presents as a system undergoing significant interaction, possibly a merger. The primary component exhibits a generally disk-like morphology, though it is highly disturbed. There's a bright, concentrated central region suggesting a prominent galactic nucleus. The overall color of the main galaxy appears yellowish-white, potentially indicating a population of older stars, although there are noticeable regions of bluer light. The disturbed morphology includes a suggestion of tidal tails or bridges emanating from the galaxy, indicative of gravitational interactions. These appear irregular, and their color suggests they contain a mix of younger and older stars. There's also the presence of features, potentially dust lanes, though this is hard to confirm due to the image quality. Overall, the galaxy is undergoing active interactions that are driving significant morphological changes.
