The galaxy presents an overall elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region appears bright and relatively unresolved, suggesting a high stellar density and potentially the presence of an active galactic nucleus. The galaxy exhibits a color gradient, transitioning from a bluer hue in the innermost regions to redder tones in the outer halo. This could be indicative of older stellar populations dominating the periphery. The galaxy appears relatively undisturbed with no obvious signs of tidal features or ongoing major mergers. The overall structure appears to be a relatively old galaxy with limited current star formation. 
