The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge. The overall color is a warm, yellow-orange hue, suggestive of an older stellar population with fewer young, massive stars. There are no discernable spiral arms or prominent dust lanes visible in this image. The galaxy exhibits a high degree of circularity, with an almost perfectly round appearance. There is no apparent evidence of any major mergers or significant tidal disturbances affecting its structure. The morphology indicates it is likely a passively evolving system with relatively low current star formation activity. The galaxy spans an estimated diameter of approximately 9 kiloparsecs.
