The galaxy presents as a generally smooth, elliptical-like structure. The core region exhibits a concentrated, bright, yellowish-white luminosity. This core transitions smoothly into an outer halo. The halo appears less concentrated with a slight blueish-green tint on the edges. There may be a hint of a disk-like structure but this is not definitive. There are no clear indications of spiral arms or major disturbances indicative of a merger event. The morphology suggests a quiescent galaxy with an older stellar population dominating the core.
