The galaxy presents a generally smooth, elliptical morphology. The core exhibits a high surface brightness, appearing nearly spheroidal with a slightly elongated shape along the major axis. The central region shows a concentration of older stellar populations, indicated by the reddish hue. Moving outwards, the galactic disk gradually fades into a diffuse halo. Faint blue light is visible in the outer regions, suggesting the presence of some younger, hotter stars. No prominent spiral arm structure or dust lanes are visible, but a slight asymmetry in the halo indicates the possibility of a minor gravitational disturbance or interaction. The galaxy's overall appearance is consistent with an early-type galaxy experiencing low levels of star formation.
