The galaxy appears to be undergoing a significant interaction, possibly a merger, as indicated by the disturbed morphology. The primary component of the galaxy exhibits a dominant, roughly ellipsoidal shape. Its central region is characterized by a high concentration of luminosity, appearing smooth and potentially representing an older stellar population.

Surrounding the central region, there are areas of bluer light, indicating regions of active star formation. These bluer areas seem more concentrated on one side of the galaxy than the other, and the areas appear to be distinct clumps. These could be indicative of tidal tails or bridges formed during the interaction or recent accretion events.

Overall, the galaxy displays a complex structure with a combination of features suggesting both an older population and ongoing star formation. The interaction has greatly disturbed the normal stellar population.
