The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a moderately elongated shape, resembling an oblate spheroid. The light profile suggests a concentration of older stellar populations, indicated by the yellowish-red hue, particularly towards the center of the galaxy. There is no obvious presence of spiral arms or significant dust lanes. Based on the observed morphology, this galaxy likely has a high bulge-to-disk ratio and minimal ongoing star formation. There is no sign of any major or minor mergers happening in this picture. The image indicates that this galaxy is fairly isolated with no other noticeable galaxies nearby, and therefore its development is likely determined by internal processes, rather than external interactions.
