The galaxy presents as a system with multiple components suggestive of an ongoing or recent interaction. Two brighter, more compact regions are the most prominent features. The southern compact region exhibits a blue-white color, possibly indicating younger stellar populations and ongoing star formation. The northern compact region appears to be a collection of distinct sources, with similar blue white colours surrounding it. Diffuse, fainter material extends from the central regions, suggesting tidal features or disrupted structures caused by gravitational interaction. The overall morphology deviates from a simple elliptical or spiral form. The galaxy exhibits significant blue light, indicating a relatively young stellar population. The galaxy displays signs of possible disturbances in its structure, possibly influenced by gravitational forces. The central concentration, along with the disturbed morphology, supports the classification of this galaxy as an interacting system.
