The galaxy presents as a single, relatively smooth object. It appears largely featureless, lacking any distinct spiral arms or a prominent disk structure. The central region exhibits a bright, concentrated core that gradually fades into an extended halo. Coloration suggests a redder overall hue, potentially indicating an older stellar population and a reduced rate of ongoing star formation. The galaxy’s morphology is generally elliptical, showing a high degree of circularity without any obvious signs of significant tidal interactions or disturbances. The size appears moderate, and no clear evidence of merging events or major disruptions is visible.
