The galaxy presents as a somewhat amorphous, elliptical structure with a central concentration of light. There is a smooth, diffused halo surrounding the core, exhibiting a slightly bluer hue. The core region appears more yellowish, potentially indicating an older stellar population. The overall shape is not perfectly spherical, showing hints of a possible disk or distorted form. There is no clear evidence of spiral arms or active galactic nuclei. There are slight irregularities suggesting minor disturbances in the galactic structure, potentially from interactions or past mergers.
