This galaxy appears to be a binary system, with two distinct galactic components engaged in what might be a gravitational interaction or an ongoing merger.

The larger component presents a diffuse, roughly elliptical morphology, with a color gradient transitioning from a yellow-orange hue at its center to a fainter, bluish white at its outer edges. This suggests a stellar population that is older and redder towards the center, with younger, bluer stars populating the outer regions.

The smaller component exhibits a more compact, circular profile. Its dominant coloration is a bright, uniform blue, indicating the presence of a significant population of young, hot stars. There is a subtle hint of a ring-like structure within this component, marked by a faint reddish hue. This could potentially signify ongoing star formation activity concentrated in a ring-like region.

There may be some evidence of tidal disturbance or connecting bridges between the two components, though the signal is weak. Further observations, particularly spectroscopic analysis, would be needed to confirm the nature of this system and the dynamics of any potential interaction.
