The galaxy presents as a moderately luminous, relatively smooth object. It exhibits a generally elliptical morphology with a high degree of central concentration. There is a hint of extended light, but no distinct spiral arm structure is discernable. The central region appears a yellow/white hue, suggesting an older stellar population, while the outer regions show a slightly bluer color, potentially indicating younger stars, though this is very subtle. No signs of tidal features or ongoing major mergers are immediately apparent. The galaxy is generally isolated.
