The galaxy presents with a complex morphology, suggestive of an interaction or merger event. Two distinct components are discernible. One component appears more elliptical in shape and exhibits a yellowish-orange hue, potentially indicative of an older stellar population with reduced ongoing star formation. The second component is bluer in color and shows a more disturbed, less defined structure. This may indicate a region of active star formation. There is a visual disturbance or bridge of material that seems to connect the two components, further supporting an ongoing interaction. Overall, the galaxy shows characteristics between smooth and featured morphology.
