The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. It is nearly circular in shape, showing no significant elongation or distortion. Its color gradient indicates a population dominated by older stars with a redder hue. There are no obvious signs of spiral arms or a prominent disk. The absence of strong blue colors suggests a low rate of recent star formation. No major ongoing mergers or tidal disturbances are apparent in this image, although there may be minor disturbances. The galaxy presents a generally undisturbed and relaxed morphology.
