The galaxy presents as a largely smooth object, likely elliptical in morphology. It appears relatively round with a possible slight elongation. The color gradient suggests an older stellar population with minimal ongoing star formation. No distinct spiral arm structure or prominent dust lanes are observed. There is no indication of a major merger event, although there might be some subtle disturbances or interactions affecting the galaxy's shape or structure. The galaxy emits strongly in the redder wavelengths, with significantly weaker emissions in the bluer wavelengths. The luminosity suggests a significant mass. Overall, the galaxy appears to be a quiescent, massive elliptical galaxy at a considerable distance.
