The galaxy presents as a centrally concentrated object with a generally smooth appearance. The morphology is consistent with an elliptical galaxy. The galaxy appears roughly circular, exhibiting only a slight elongation. There is a distinct color gradient, with the core exhibiting a yellowish hue and the outer regions fading into a bluer tint. No prominent spiral arms or dust lanes are discernible. There is no evident major disturbance suggesting a major merger. The galaxy is likely a fairly massive system. The faint bluer outer regions suggest ongoing but low-level star formation activity.
