The galaxy presents as a smooth, elliptical structure with a concentrated central bulge that appears mostly spheroidal. The core exhibits a notable yellowish-orange hue, suggesting an older stellar population dominated by red giants. A subtle, bluish halo surrounds the core, potentially indicative of some younger, bluer stars, or possibly an artifact of the imaging process. There is no discernible disk structure or spiral arm features visible. The overall smooth appearance and high central concentration supports a classification as an early-type galaxy, likely an elliptical. There appears to be a small concentration of stars on the edge of the halo. There do not appear to be any major mergers happening within the galaxy. 
