The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge and a diffuse halo that diminishes in intensity with increasing radius. There is evidence of a faint arm-like structure extending outward from the main body, giving it a slightly perturbed appearance suggesting minor gravitational interactions with a possible companion. The color profile indicates a higher concentration of older stellar populations. There are a few bluer areas as well, with faint spiral-arm-like appendages to the galaxy.
