The galaxy appears to be a relatively compact object, exhibiting a smooth, spheroid morphology. There is an indication of some distortion, possibly a minor disturbance in its structure. The light distribution suggests a central bulge with some extension, but it is somewhat featureless. There is no strong evidence of spiral arms or a well-defined disk. The galaxy is not perfectly circular, appearing slightly elongated in shape. It does not show signs of a major merger, however, there is a subtle irregularity in shape, possibly indicating a past interaction or minor ongoing merger event.
