The galaxy presents a flattened, elliptical morphology. Its light is distributed smoothly, with a central region exhibiting higher surface brightness. The core is a yellow-white hue, surrounded by a bluer, diffuse halo. The galaxy does not display any prominent spiral arm structure or evidence of a distinct disk. The overall color suggests a population of older stars, although there is evidence of some ongoing, low-level star formation in the bluer outer regions. The galaxy's morphology is somewhat irregular, possibly due to a past interaction or merger.