This galaxy appears to be a relatively smooth, elliptical-like structure. Its overall color is a yellowish-orange hue, suggesting an older stellar population. It exhibits a high degree of central concentration with a gradual fade toward the edges. There is a slight elongation in its shape. No distinct spiral arms or dust lanes are visible. There is no evidence of any major merging events or significant tidal disturbances. Overall the galaxy exhibits properties consistent with a relatively passive, evolved galaxy.
