The galaxy presents as a somewhat elongated, ellipsoidal structure with a distinct central bulge. The core region exhibits a bright, concentrated luminosity, appearing yellowish. Moving outward from the core, the light gradually diffuses, transitioning into a more greenish-yellow hue. The outer regions appear less defined, fading into the background. The galaxy appears relatively smooth with little or no strong spiral arm structure. The overall morphology suggests a galaxy with an intermediate disk presence. The light profile indicates a centrally concentrated system, where the bulge is significantly brighter than the disk. Faint color variations might be indicative of moderate star formation activity within the disk.
