The galaxy presents a generally smooth, elliptical morphology. Its light profile exhibits a high degree of central concentration, appearing nearly circular in shape. The core region is bright, with a color gradient trending towards slightly bluer hues. This bluer coloring may be due to a small population of hot, young stars. There are no prominent dust lanes, spiral arms, or other clear features of a disk galaxy readily visible in this image. Subtle indications of minor disturbance cannot be ruled out but appear unlikely. Overall, the galaxy appears to be a relatively undisturbed, spheroidal system. Its estimated size suggests that it is a relatively small system for its redshift.
