The galaxy presents as a relatively smooth, elliptical structure with a centrally concentrated luminosity profile. The core region appears to be yellowish, indicating an older stellar population. Moving outward from the core, the galaxy exhibits a gradual fading of light intensity. There is little to no evidence of spiral arms or distinct features typically associated with disk galaxies. The overall shape is more rounded than elongated, though not perfectly spherical. No prominent tidal tails or distortions suggestive of recent major mergers are immediately apparent. The outer regions are characterized by a bluer hue.
