The galaxy appears as a relatively compact object with a generally smooth morphology. It exhibits a somewhat elliptical shape, appearing more rounded than elongated. There is evidence of a bulge-like structure, with a brighter central region that fades into the surrounding galactic disk. The galaxy displays a color gradient, with the central regions appearing more reddish, possibly indicating an older stellar population or significant dust obscuration. The outer regions show a slight hint of bluer colors, suggestive of younger stars or ongoing star formation. There is a potential faint tidal tail that could be another galaxy being consumed in the early stages of a merger. The main body of the galaxy appears undisturbed, with no strong signs of ongoing major merging activity. 
