The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. It appears largely spheroidal in shape, with a high degree of radial symmetry, lacking any obvious spiral arm structure or prominent disk features. There is a subtle color gradient, exhibiting a more yellow-orange hue in the core, which fades to a dimmer redder tone at the outer regions, suggesting an older stellar population predominating throughout. The relative smoothness in surface brightness distribution suggests it is an elliptical galaxy. No active galactic nucleus is visually apparent, and there is no evidence of ongoing major merging activity. There's a subtle suggestion of some minor disturbance of material, though this is difficult to confirm.
