The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. The central region exhibits a bright, nearly unresolved core that diminishes in intensity outwards. The isophotes appear elliptical with an estimated axis ratio of approximately 0.8, suggesting a flattened shape. There is a subtle color gradient visible, with the central core appearing slightly bluer than the outer regions, potentially indicating variations in stellar populations or dust content. No distinct spiral arms or prominent features are discernible in the image. Overall, the galaxy appears relatively undisturbed.
