The galaxy presents a relatively smooth, elliptical morphology. Its core appears bright and concentrated, exhibiting a yellowish-white hue, which may indicate an older stellar population and/or significant dust obscuration. The disk component is observed at an oblique angle, creating an elongated shape. The outer regions of the galaxy fade gradually, suggesting a diminishing stellar density with increased radial distance from the core. Subtle color gradients are perceptible, with the inner regions presenting a more yellowish tint shifting toward a bluer hue in the outer disk, suggesting some level of ongoing star formation. No distinct spiral arm structures are visible in this image, supporting its generally smooth and elliptical classification. Overall, the galaxy appears to be a reasonably evolved system with a mix of stellar populations.
