The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The color profile suggests an older stellar population, with a dominant yellowish hue characteristic of evolved stars. There is little evidence of spiral arm structures or significant dust lanes within the visible spectrum. The overall structure appears relaxed and relatively undisturbed, indicating a lack of recent major merger events. A subtle asymmetry in the outer halo might suggest a minor interaction or past accretion event.
