The galaxy appears as a smooth, centrally concentrated object with a slightly elliptical morphology. The core exhibits a bright, yellowish-white hue, indicating a substantial population of older stars. Moving outward from the center, the color shifts to a more greenish-yellow, suggesting a gradual transition in stellar populations and potentially a small amount of ongoing star formation in the outer regions. The overall structure lacks any prominent spiral arms or distinct features, indicative of a relatively undisturbed system. The galaxy exhibits a relatively uniform distribution of light, with a gentle falloff in intensity from the core to its outer edges. There is no evidence of any major tidal disturbances or ongoing mergers.
