The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits an approximately elliptical morphology, with a diffuse halo. The core region displays a warm hue transitioning to cooler tones in the outer regions. Evident is a dominant spheroid component with limited discernible structure in the form of spiral arms or a prominent disk. The smooth appearance suggests a lack of significant recent merger activity or major disturbances. Color gradients indicate older stellar populations are primarily concentrated in the central bulge, while younger stars may be more sparsely distributed throughout the broader galactic structure. There does not appear to be a substantial amount of on-going star formation.
