This galaxy presents a largely smooth morphology. The light is concentrated, with a bright, nearly circular core exhibiting a yellowish-orange hue. There is a fainter, diffuse, greenish halo extending outwards from the core. The halo lacks any defined spiral arm structures, or significant dust lanes, appearing relatively homogeneous. The overall impression is that of a fairly undisturbed system. The apparent roundness suggests a minimal inclination relative to our line of sight. There are no visual indications of a major ongoing merger event, though subtle irregularities in the outer halo cannot be ruled out based on this image alone.
