The galaxy appears as a centrally concentrated object. The core region exhibits a bright, relatively uniform blue color profile, suggesting a population of hot, young stars, or possibly AGN activity. The surrounding halo transitions to a greenish hue further out, possibly indicative of older stellar populations or dust attenuation. There are some traces of red concentrations within the halo, which could point to star forming regions. There's no strong indication of spiral arm structure or a distinct disk; the galaxy appears more spheroidal in shape. Overall, the light distribution appears relatively smooth, but there are hints of morphological disturbances in the halo.
