The galaxy presents as an elliptical morphology, largely featureless and smooth in appearance. A centrally concentrated bulge dominates the light profile, fading gradually outward. The core exhibits a yellowish-orange hue, suggesting an older stellar population and minimal ongoing star formation. There is no clear evidence of spiral arms or a distinct disk component. The outer regions appear more diffuse, lacking sharp edges, which points towards a quiescent state. The overall round shape indicates a relaxed dynamical state. There is no strong evidence of tidal features or major disturbances suggesting a recent merger event. The galaxy shows a color gradient with the inner region displaying redder hues, indicating a difference in stellar populations and a suppression of star formation activity. 
