The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, diffuse glow that diminishes gradually outward. There is an absence of discernible spiral arm structures or prominent dust lanes. The overall color is slightly red-shifted, suggestive of an older stellar population. Faint, extended halo features are barely discernable but suggest a moderate degree of spheroidal symmetry. There appear to be no signs of recent major mergers or tidal disturbances, although minor asymmetries cannot be ruled out at this resolution. The object appears relatively undisturbed.
