The galaxy presents a primarily smooth, elliptical morphology with a high degree of central concentration. Its shape is approximately in between round and elliptical, slightly elongated along its major axis. There is a bright central bulge or core, exhibiting a yellowish-white hue, suggesting a population of older stars. The outer regions fade gradually into a diffuse halo, tinged with blue. This bluer component possibly indicates regions of more recent star formation, though subdued. There is no strong evidence of spiral arms or a distinct disk structure. No significant signs of major mergers or strong tidal disturbances are visible in the immediate vicinity. Faint minor disturbances cannot be fully ruled out due to image resolution.
