The galaxy presents as a centrally concentrated, relatively smooth object. The core exhibits a yellowish hue, suggesting an older stellar population dominating the inner regions. The outer regions display a gradient towards a greenish-blue color, potentially indicative of younger, hotter stars and ongoing star formation in the outer disk. There are no readily apparent spiral arm structures or bar features visible in this image. The overall morphology appears close to elliptical, although it has a moderately high roundness. There is no visually clear indication of any major merger activity or significant tidal disturbances. The galaxy seems relatively undisturbed.
