The galaxy presents a lenticular morphology, exhibiting a smooth, elliptical light distribution characteristic of S0 galaxies. The central bulge appears prominent and displays a yellowish hue, suggesting an older stellar population. A faint, flattened disk surrounds the bulge, oriented at an angle relative to the observer's line of sight. Hints of bluer light are observed in the outer regions of the disk, indicating the presence of some younger stars or ongoing, albeit subdued, star formation. There is no evidence of strong spiral arm structure, but subtle irregularities in the disk's light distribution could suggest minor disturbances or interactions in the past. The overall structure of the galaxy is fairly regular, with no major signs of ongoing mergers or strong tidal interactions.
