This galaxy appears to be a relatively large, disk-shaped system viewed at an oblique angle. The light distribution suggests a centrally concentrated bulge or core region that gradually fades into a more diffuse disk. The galaxy exhibits an overall smooth appearance, with a hint of spiral structure. The color profile indicates a higher concentration of older stellar populations and potentially dust extinction in the central regions, giving it a redder hue. Progressing outwards, the disk may contain younger, bluer stars. There are no obvious signs of major interactions or mergers, and the galaxy exhibits fairly regular morphology. Minor disturbances cannot be ruled out.
