The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. It displays a near-perfect circular morphology, with no discernible disk-like features or spiral arms. The light is dominated by a yellowish-white hue, indicative of an older stellar population. There is a slight color gradient with the core of the galaxy appearing whiter than the outer edges. There is no visual evidence of ongoing major merger activity or significant tidal disturbances. Any faint, featured light likely resides close to the central bulge.
