The galaxy presents as a moderately bright, relatively smooth object. Its morphology appears to be primarily elliptical, exhibiting a high degree of central concentration with a gradual decrease in luminosity towards its outer regions. There is a slight elongation visible, deviating minimally from a perfect circular shape. Subtle color gradients are detectable, suggesting potential variations in stellar populations across the galaxy. Overall, the light appears to be on the redder side. There is no apparent spiral structure, bar, or dust lane. Evidence of tidal disturbances is not immediately obvious. The galaxy appears undisturbed, with no indication of a recent major merger event.
