The galaxy appears as a relatively smooth, elliptical structure. The light is concentrated towards the center, indicating a dense galactic nucleus. There is a discernible color gradient from the center outwards, with the core exhibiting a yellow hue that gradually shifts towards redder tones in the outer regions. The overall morphology suggests an evolved system with little to no evidence of significant star formation activity in the recent past. No distinct spiral arms or disk-like features are visible, lending further support to the classification as an elliptical galaxy. There are no obvious signs of ongoing mergers or tidal disturbances. The galaxy appears to be relatively isolated and undisturbed.
