The galaxy presents as a system with apparent morphological disturbances, possibly indicative of an ongoing or recent merger event. There appear to be multiple interacting components, with a primary, somewhat amorphous central region displaying a blueish hue, potentially reflecting ongoing star formation. Evident are diffuse extensions or tidal features emanating from the core, further suggesting gravitational interaction. Overall, the galaxy's structure deviates significantly from a regular elliptical or spiral morphology, instead presenting an irregular, disturbed form. Color variations throughout the galaxy imply differing stellar populations or dust distribution patterns.
