The galaxy presents as a centrally concentrated, relatively smooth object. Its morphology appears elliptical, exhibiting a high degree of circularity in its overall shape. There is minimal evidence of spiral arm structure or significant disk features. The light distribution suggests a bulge-dominated system with a gradual falloff in intensity from the core outwards.  Color gradients are subtle, with the core region showing a slightly more yellow hue compared to the outer regions. There are no obvious signs of major mergers or significant tidal disturbances within the galaxy’s structure, though a possible minor disturbance cannot be ruled out due to image resolution.
