The galaxy exhibits a complex morphology, appearing as a multi-component system. A dominant central region is visible, exhibiting a slightly elongated shape. This central component demonstrates a generally smooth texture with a possible hint of a disk-like structure. The galaxy's color profile suggests a mix of stellar populations, with a central concentration of bluer wavelengths possibly indicating recent star formation. 

Connected to the main body of the galaxy, a distinct secondary component can be seen. This component is more compact and exhibits a redder color profile, potentially indicating an older stellar population or significant dust obscuration. 

The overall structure suggests a possible ongoing or recent interaction or merger event. The asymmetry in the distribution of light and color, along with the presence of a distinct secondary component, supports this hypothesis. Further analysis, including higher-resolution imaging and spectroscopic data, would be beneficial to confirm the nature of the interaction and the properties of the individual components.
