The galaxy appears to be a relatively round, elliptical galaxy. Its core is very bright and concentrated, with the luminosity fading gradually toward the outer edges. The galaxy's color suggests an older stellar population, as it appears generally yellowish-white, lacking prominent blue regions typically associated with active star formation. There are no distinct spiral arms or other prominent features usually indicative of a disk galaxy, though there is a faint, small irregular-shaped object to the lower right that could be a tidal stream or other disrupted feature. The overall structure suggests the galaxy is relatively undisturbed, with no major signs of recent mergers or interactions.
