The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. It presents with a generally round shape, with only slight deviations from perfect circularity. There is a distinct color gradient visible, transitioning from a yellowish, brighter core to a redder, fainter outer halo. This color gradient suggests a radial variation in stellar populations, with older, redder stars dominating the outer regions.

No prominent spiral arms or disk-like features are discernible. The galaxy lacks significant dust lanes or other signs of recent or ongoing star formation, indicative of a relatively quiescent galaxy with low star formation rates. The overall structure suggests a relatively relaxed system, without obvious signs of recent mergers or major disturbances. The light distribution is fairly even across the galaxy, with no clear irregularities or lumpy structures.
