The galaxy appears to be an elliptical galaxy. It exhibits a smooth, diffuse light distribution with a high degree of central concentration. The overall shape is elongated, approaching a cigar-like morphology. There is no obvious spiral arm structure or dust lanes visible. The color suggests an older stellar population. The galaxy appears relatively undisturbed, showing no significant signs of ongoing or recent major merger activity, though there is a small likelihood of a minor disturbance influencing the system. The core displays a yellowish hue, potentially indicating a large population of older, cooler stars. The galaxy fades smoothly towards its outer edges, implying a gradual decrease in stellar density away from the nucleus.
