The galaxy presents as a largely featureless elliptical, exhibiting a smooth, concentrated light profile. Its shape is roughly in between round and elongated. The central region displays a high surface brightness, with a yellowish hue, likely indicating an older stellar population dominating the core. The outer regions are less luminous and display a hint of greenish blue, possibly representing a small degree of recent or ongoing star formation in the extended disk. There is no prominent evidence of spiral arms or other significant morphological features typically associated with disk galaxies, nor are there any obvious signs of tidal disturbances or ongoing mergers, indicating that this is a relatively isolated system.
