The galaxy presents as a nearly circular, concentrated light source, exhibiting a smooth, featureless morphology. The galaxy appears to be a single structure, with no visible signs of merging activity or major disturbances. The central region is noticeably brighter, indicating a dense concentration of stars or an active galactic nucleus. The outer regions gradually fade into the background, showing a smooth transition in luminosity. There's a slight bluish hue in the central regions, possibly indicating recent star formation. Overall, the galaxy's morphology suggests a relatively evolved system.
