The galaxy presents as a centrally concentrated, elliptical or lenticular system. The central bulge exhibits a smooth, diffuse light profile, suggesting an older stellar population. There is a subtle color gradient, with the core appearing slightly bluer than the outer regions, potentially indicating some ongoing, albeit subdued, star formation in the nucleus. Faint, extended light emanates from the core, forming a halo-like structure. No prominent spiral arms or distinct dust lanes are visible. The overall shape is generally rounded, with a slight elongation. There is no strong evidence of tidal disturbances or major mergers in the immediate vicinity, but a minor perturbation cannot be entirely ruled out.
