The galaxy presents as a slightly elongated, lenticular or early-type spiral system, with a smooth, concentrated central bulge region that appears yellowish-orange in color. A faint, blueish disk surrounds the central bulge. The luminosity decreases smoothly from the core to the outer edges, suggesting a high degree of symmetry. Faint spiral arms or other distinct structures are not obvious in the image, though some subtle irregularities in the disk's color and brightness distribution may indicate regions of ongoing or recent star formation. The overall morphology suggests an evolved galaxy with a significant stellar mass. There is no evidence of a major ongoing merger event, although some minor disturbances or tidal features cannot be ruled out based on the image alone.
