The galaxy presents as a relatively compact structure with an apparent moderate angular size. Overall the morphology shows characteristics indicative of a merger event. The primary structure, near the center of the image, appears mostly smooth with a bright, relatively concentrated core region exhibiting a bluish hue, possibly indicating a population of younger, hotter stars. 

A separate structure is observed in close proximity. This smaller structure is a yellow-orange color. The irregular shape suggests interaction and tidal distortion caused by gravitational forces between the objects. Furthermore, a fainter, less distinct concentration of light is located below the main body, potentially indicating a third interacting component or the remnant of tidal debris. 
