The galaxy presents as a flattened, elliptical morphology with a bright, concentrated central bulge that emits a yellowish light, possibly indicating an older stellar population. The outer regions display a more diffuse and fainter light, suggesting the presence of a stellar disk, with hints of bluer colors mixed in, perhaps indicating some ongoing star formation. The overall structure appears relatively undisturbed, showing no obvious signs of tidal interactions or major mergers, although there is a slight suggestion of disturbance in the faint outer regions. The galaxy is moderately inclined with respect to our line of sight, allowing a good view of the disk-like structure.
