The galaxy presents as an elliptical form, with a noticeable concentration of light toward the center. The central bulge appears smooth and lacks distinct structural features. The light distribution suggests a relatively old stellar population, indicated by the yellowish hue. The galaxy is somewhat elongated, appearing more "in-between" than completely round. There is no obvious indication of active merging or major disturbances within the galaxy's morphology, although slight asymmetries could indicate minor interactions in its recent past. The outer regions gradually fade, showing a smooth decline in stellar density from the core.
