The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, relatively uniform luminosity profile that decreases gradually outwards. Faint blue tinges are visible, suggesting some recent star formation although it is dominated by an older stellar population. The galaxy appears mostly undisturbed, without any major signs of ongoing mergers or tidal interactions. The galaxy is generally round in shape with no obvious disk-like structure or spiral arms. There is the possibility of a companion galaxy to the lower left.
