The galaxy presents as a relatively smooth and amorphous structure. Its light distribution is centrally concentrated with a gradual decline in intensity towards the outer regions. The morphology appears to be more elliptical than spiral, displaying a somewhat elongated shape with axial asymmetry. There is a slight color gradient visible, trending from a bluer core to redder outskirts, suggesting a radial variation in stellar populations and/or dust content. The absence of prominent spiral arms or a distinct disk indicates a lack of significant current star formation, however there may be some ongoing star formation, but at a low rate. There is no noticeable evidence of recent mergers or major disturbances affecting its overall structure.
