The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. There is no discernible spiral arm structure or bar. The core exhibits a yellowish-white hue, suggesting an older stellar population, while the outer regions of the galaxy show a gradual color gradient toward a bluer tint. The overall form is mostly round, with no obvious signs of major tidal interactions or significant morphological disturbances. There appears to be little to no evidence of strong dust lanes or prominent star-forming regions based on the smoothness and lack of significant color variations.
