The galaxy presents as a diffuse, irregular structure with a prominent central region of intense blue luminosity. The overall shape appears elongated, with a slight tilt relative to the line of sight. There is evidence of disruption or interaction, possibly indicating an ongoing or recent merger event. The brighter blue light suggests active star formation, particularly concentrated within the central region and potentially extending into some fainter outer regions. The outskirts are less well-defined, exhibiting a more amorphous, fainter halo.
