This galaxy exhibits a somewhat amorphous structure with a centrally concentrated luminosity profile. The primary color is a bluish-white, suggesting the presence of a younger stellar population and ongoing star formation, particularly towards the core. Fainter extended regions show disturbed morphology indicative of a potential recent or ongoing interaction. These disturbances include faint tidal tails and some disrupted arms. There appear to be pockets of intense star formation scattered throughout the galaxy. Despite the disturbances, there remains some underlying smoothness to the central region, it looks like it could be disk galaxy. Overall, the galaxy appears to be in a dynamic state, influenced by gravitational interactions, with an estimated mass lower than our own Milky Way.
