The galaxy presents an elliptical morphology, elongated along its major axis, with a high degree of smoothness. Its central region exhibits a concentrated luminosity, transitioning to a more diffuse, fainter halo. Color gradients are subtle, with a slightly bluer hue in the outer regions suggesting younger stellar populations compared to the central, yellower core. No distinct spiral arm structures or significant dust lanes are visible. A small, faint disturbance is seen in the upper-right part of the galaxy, but no signs of major merger activity are obvious.
