The galaxy presents as a smooth, centrally concentrated object with a generally elliptical morphology. The light distribution exhibits a high degree of radial symmetry, lacking any readily discernible spiral arm structure or strong irregularities. The core region displays a bright, concentrated luminosity, suggesting a significant stellar density. Moving outward from the center, the luminosity gradually diminishes, creating a diffuse halo effect. The overall color is yellowish. The image suggests this is a relatively undisturbed galaxy with no major ongoing merger activity. There is no evidence of tidal tails or strong morphological distortions. 
