The galaxy presents as a concentrated, ellipsoidal structure with a smooth, diffuse light distribution. A bright central bulge dominates the core, exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. The galaxy appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The outer regions exhibit a gradual decrease in luminosity, fading into the background. There may be faint, subtle color variations within the galaxy's halo, shifting toward slightly bluer tones at the periphery, suggesting some ongoing, albeit minimal, star formation. Overall, the morphology suggests an elliptical galaxy with a quiescent nature.
