The galaxy presents as an apparent merger or interaction of multiple components. One primary component appears relatively smooth and elliptical, exhibiting a yellow-red hue indicative of an older stellar population or significant dust obscuration. Another component shows a bluer color, possibly indicating on-going star formation. The morphology suggests moderate-to-high stellar mass, with the potential for moderate star formation activity. There appears to be some tidal distortion or extended features suggesting an interaction with another galactic body. The relative prominence of the redder component suggests it could be a more evolved system compared to the bluer component, or the reddening of the bluer object could simply be due to dust. Overall the galaxy appears relatively compact, yet possibly undergoing complex evolutionary processes.
