The galaxy exhibits an elliptical morphology, appearing largely smooth and featureless. It presents a concentrated central bulge that gradually fades into an extended halo. The color gradient transitions from a yellowish hue in the core to a greenish tint in the outer regions, which may indicate variations in stellar populations or dust content. The lack of spiral arms or significant dust lanes suggests a relatively quiescent state. The galaxy appears to be fairly isolated with no nearby galaxies.
