The galaxy appears as an elliptical structure, exhibiting a smooth, symmetrical morphology. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. The core exhibits a yellowish hue, suggesting a population of older stars. There is a lack of distinct spiral arm structures or prominent dust lanes, characteristic of elliptical galaxies. A faint, smaller structure is visible towards the lower left quadrant, which could possibly be a minor tidal disturbance or a smaller interacting galaxy. The overall structure appears relatively undisturbed, indicating a stable, evolved system.
