The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth light distribution. The core region displays a yellowish hue, suggesting an older stellar population. Surrounding the core, the galaxy fades into a more diffuse disk. Within this disk, bluer colors are visible, indicating pockets of more recent star formation. There are some slight indications of structural asymmetry, potentially arising from minor gravitational interactions. Overall the shape is highly rounded. There doesn't appear to be any significant signs of major disturbances from galactic mergers.
