The galaxy presents as a somewhat diffuse object, exhibiting an irregular morphology. Two distinct, brighter, and more compact components appear to be present, with a faint, diffuse halo encompassing both. The color gradient suggests variations in stellar populations or dust content, with the brighter regions exhibiting warmer hues, likely indicating younger stellar populations or intense star formation. The overall structure suggests a possible interaction or merger in progress, as there are deviations from a simple elliptical or spiral form. There is some evidence of disruption within the halo of the galaxy, further supporting the hypothesis of a merger. 
