The galaxy appears as a centrally concentrated object with a relatively smooth overall morphology. There is a slight extension in the redder wavelengths towards the lower right. The central region exhibits a relatively bright, unresolved core, surrounded by a more diffuse halo. The galaxy is largely spheroidal in appearance, showing minimal evidence of spiral arm structure or significant disk-like features. The light distribution appears relatively even across the object. There is no clear evidence of a major ongoing merger, though minor disturbances cannot be ruled out based solely on this image. The color indices suggest ongoing star formation.
