The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated morphology. The overall color profile suggests an older stellar population, trending towards a redder hue. There is a subtle elongation present, but the overall structure lacks prominent features such as spiral arms or a distinct disk. A slight asymmetry or minor disturbance might be present, possibly suggestive of a past interaction or minor merging event. The concentration of light indicates a significant central bulge. The galaxy is relatively compact in angular size.