The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. It presents a highly concentrated central bulge, with a gradual decrease in luminosity outwards. The color gradient suggests an older stellar population dominating the galaxy, with a yellowish hue at the core transitioning to a slightly redder, fainter halo. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy shows a high degree of circular symmetry. There are no indications of ongoing major mergers or tidal disturbances, although some minor asymmetries may be present in the outer regions. 
