The galaxy appears as a bright, centrally concentrated object, exhibiting a smooth morphology. The core region is intensely luminous, showing a yellow-orange hue suggestive of an older stellar population. The light gradually diminishes outwards from the center, with the outer regions displaying a more diffuse and indistinct boundary. There are no visible spiral arms or prominent dust lanes, indicating a lack of significant recent star formation. The overall shape is generally round, with only subtle deviations from perfect circularity. There is no visual evidence of ongoing mergers or major tidal disturbances in this image.
