The galaxy presents a generally smooth and elliptical appearance, exhibiting a high degree of central concentration with a bright, unresolved core. The overall color profile suggests a population dominated by older stars, with a weak presence of bluer, younger stars. The galaxy appears largely undisturbed, showing no obvious signs of major mergers or significant tidal interactions. Faint indications of a possible disk structure are present, though no clear spiral arms are visible. There is a hint of possible minor disturbance in the outer regions, though most of the galaxy appears generally uniform and consistent with that of a lenticular or elliptical morphology.
