The galaxy presents as a fairly smooth, elliptical structure. It is yellowish-white in color, suggesting an older stellar population and a relatively low rate of current star formation. The light distribution appears concentrated towards the center, with a gradual decrease in luminosity towards the edges. There is no evidence of strong spiral arms or a prominent disk component. The overall shape is somewhat elongated, leaning towards an in-between shape, rather than perfectly round or cigar-shaped. There is no obvious indication of any major ongoing mergers or significant tidal disturbances. The galaxy's apparent integrated magnitude indicates it is fairly bright and massive at its given redshift.
