The galaxy appears as a centrally concentrated, relatively smooth structure. It exhibits a somewhat elliptical morphology, not perfectly spherical. There appears to be a slight flattening along one axis. The color distribution suggests a dominant population of older stars, with a hint of bluer colors in the central region, possibly indicating some ongoing, but low-level star formation. There is no obvious spiral structure or strong evidence of a prominent disk. However, a hint of disk structure cannot be ruled out. There is a lack of any distinct tidal features or clear signs of a major ongoing merger event, although some subtle disturbances in the outer regions may suggest a minor interaction in its past or some internal dynamics. The overall light distribution is centrally concentrated.
