This galaxy presents as a largely smooth, elliptical structure. It displays a fairly concentrated central bulge, fading into an extended halo. The color appears to be consistent across the galaxy, exhibiting a slightly redder hue, suggestive of an older stellar population and relatively low ongoing star formation. There's little evidence of distinct spiral arms or a significant disk component. The galaxy exhibits a high degree of roundness in its overall shape. There appears to be no prominent morphological disturbances, such as tidal tails or signs of recent mergers. Its estimated size is a few kiloparsecs in radius. The object is relatively bright, implying a high luminosity despite the lack of active star formation. The estimated redshift places this galaxy at a considerable cosmological distance.
