The galaxy presents as a centrally concentrated, smooth object with a moderately elliptical morphology. The core region exhibits a diffuse, yellowish hue, suggesting an older stellar population. There may be a faint blue light signature in the galaxy disk. The galaxy appears to be experiencing some level of interaction or disturbance; it has a tail-like shape and could possibly be merging with multiple other objects or dwarf galaxies. These faint structures are extended and ill-defined, which suggests a fairly well advanced degree of interaction or an unusual structure.
