The galaxy presents a smooth, largely featureless morphology. It appears to be elliptical, with a generally round shape, though it is difficult to discern subtle deviations from perfect circularity at this resolution. There is a noticeable color gradient, with the central region appearing brighter and bluer, suggesting a concentration of younger, hotter stars in the galactic nucleus. The outer regions of the galaxy exhibit a redder hue, indicating an older stellar population. The overall light distribution is relatively smooth and centrally concentrated, with no obvious signs of spiral arms or a prominent disk. There are no visual indications of any ongoing major mergers or significant tidal disturbances.
