The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core, transitioning to a fainter, more diffuse outer halo. There is evidence of a subtle color gradient, shifting from a warmer, reddish-yellow hue in the center to a cooler, greenish-blue tint toward the periphery. While the overall structure appears undisturbed, there is a slight asymmetry, possibly indicating minor tidal interactions or internal dynamic processes. The lack of prominent spiral arms or dust lanes suggests a relatively quiescent star formation rate. The galaxy displays an intermediate roundness, deviating neither strongly towards a circular nor a highly elongated shape.
