The galaxy presents as a merging system, with two distinct components. The primary component appears relatively smooth and elliptical in shape, exhibiting a yellowish-red hue suggestive of an older stellar population. The secondary component, positioned nearby, displays a slightly greener color, indicating the presence of younger, hotter stars and potentially ongoing star formation. There is evidence of tidal disturbance, with possible faint extensions or distortions around the interacting components. The system's morphology is clearly disturbed, characteristic of a galaxy merger in progress.
