The galaxy presents a dual-component structure. The primary component exhibits a relatively smooth morphology with a somewhat round appearance. Its color profile leans towards the redder end of the spectrum, suggesting a population of older stars and potentially a lower rate of current star formation. 

Adjacent to this is a secondary component that appears distinctly bluer. This may suggest the presence of a region with active star formation, populated by hotter, younger stars. The overall shape is not well-defined, possibly indicating a disturbed or irregular structure. There are hints of minor tidal disturbances, though not pronounced.

The interaction between the two components seems to be influencing the overall morphology of the system. The bluer component is less distinct.
