The galaxy presents an overall irregular morphology. The central region exhibits a bright, compact core, with a dominant blue-white coloration, suggesting a population of hot, young stars or active galactic nucleus activity. Surrounding this central concentration, there is a fainter, more diffuse halo. The light within this extended region shifts from a predominantly blue color near the core to a greener hue further outward. This color gradient could indicate a transition in stellar populations or differential dust extinction. There appears to be a possible tidal tail or disrupted arm extending from the main body of the galaxy.
