The observed galaxy exhibits a complex morphology. Its light profile suggests a primarily irregular structure with a slight central concentration, though not indicative of a prominent bulge. There is evidence of tidal features suggesting a recent or ongoing interaction or merger. One discerns faint plumes and wisps extending outwards from the main body of the galaxy. These are not symmetrical; instead they are concentrated to one side. The galaxy's color indices suggest ongoing star formation within the object, particularly within these extending plume structures, which appear to be a bluer hue.
