The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. Its shape is more cigar-like than circular, and the galaxy shows a distinct color gradient, appearing more yellow or golden toward the center and subtly bluer at the edges. There is no apparent spiral structure, nor are there any strong signs of ongoing mergers or major disturbances. Based on the galaxy's color, we can infer that it may be comprised of older, more evolved stellar populations. This galaxy has an estimated size of approximately 7 kiloparsecs.
