The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated core region dominates the luminosity profile, exhibiting a yellow-white color. The radial light distribution appears to decrease smoothly from the core outwards, forming a halo with a slightly bluer hue, hinting at the presence of younger stellar populations in the outer regions. No distinct spiral arms or bar structures are visible in this image. There are no signs of major tidal disturbances or ongoing mergers, though minor irregularities in the outer halo cannot be ruled out based on this single image. The galaxy appears relatively isolated within its immediate field.
