The galaxy presents as a moderately sized, elongated structure, likely a lenticular or elliptical type. Its morphology is dominated by a smooth, relatively featureless appearance, with a high degree of central concentration. There is a distinct color gradient, transitioning from a yellowish-white core to a redder, more diffuse outer halo. This suggests an older stellar population is predominant. The galaxy lacks apparent spiral arm structures or distinct dust lanes. Its overall shape is highly flattened. The galaxy appears relatively undisturbed, with no obvious signs of recent mergers or tidal interactions.
