The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The overall shape is elongated, with a major axis noticeably larger than its minor axis. There is a pronounced color gradient within the galaxy. The central region displays a yellowish hue, possibly indicating an older stellar population. Progressing outwards from the center, the color shifts towards bluer tones, which may indicate more recent star formation in the outer regions. The edges of the galaxy appear diffuse, lacking a sharp, well-defined boundary, which is consistent with a gradual decrease in stellar density. No prominent spiral arm structures or dust lanes are discernible in the image. The galaxy appears relatively undisturbed, without obvious signs of recent major mergers or tidal interactions.
