The galaxy appears to be an elliptical galaxy, exhibiting a high degree of smoothness in its overall structure. It shows no distinct disk features or spiral arm morphology. The galaxy's shape is predominantly round. The color gradient suggests a higher concentration of older stellar populations in the core, which are likely to be redder in color. There is a slight color change to blue toward the edge, this could be due to recent interactions causing the creation of new, younger stars. There is no visual evidence of significant ongoing merger activity or tidal disturbances. The galaxy appears relatively isolated and undisturbed.
