The galaxy presents as an elliptical morphology, exhibiting a largely smooth, featureless appearance. The central region displays a concentrated, bright core which fades gradually into the outer regions of the galaxy. Colors transition from a yellow-orange hue in the nucleus to a blue-green tint toward the outer edges, perhaps indicating the presence of some younger stars in the outer regions, or perhaps the result of instrument response and redshifting. The overall roundness suggests the galaxy is viewed close to face-on, with no significant evidence of a disk structure or spiral arms. There is a slight indication of a minor disturbance on the left side of the galaxy, potentially indicating minor tidal interactions, but the overall structure appears relatively undisturbed and stable.
