The galaxy presents as a centrally concentrated, smooth, and relatively featureless system. Its morphology appears largely elliptical, exhibiting a high degree of sphericity. The light profile smoothly transitions from a bright core to a fainter outer halo, with no obvious spiral arm structure or prominent dust lanes visible. There is a subtle color gradient, with the central region appearing slightly more yellow/orange, suggesting an older stellar population. No significant tidal features or distortions are apparent, indicating the absence of recent major mergers or interactions. There may be the beginning stages of minor disturbances as light shifts in the image.
