The galaxy appears as an elliptical-like structure, exhibiting a centrally concentrated luminosity profile that gradually fades towards its outer regions. The core region of the galaxy displays a warmer, yellowish color, suggesting an older stellar population. The outer regions, in contrast, have a distinct bluish tint indicating the presence of younger, hotter stars. Overall, the morphology appears relatively smooth, with only slight evidence of any disk-like or spiral arm substructure. The galaxy exhibits a high degree of symmetry, lacking any obvious signs of recent major mergers or tidal disturbances, although a minor disturbance cannot be ruled out. The galaxy is moderately inclined relative to our line of sight.
