The observed galaxy presents a mostly smooth morphology. The shape appears to be somewhere between round and elliptical. The central region is noticeably brighter, suggesting a concentration of stellar mass or possibly an active galactic nucleus. There are subtle hints of faint, diffuse structures extending outward from the central region that could indicate faint stellar arms. The overall color is a warm yellow. These features may indicate either a spheroidal galaxy or a relatively undisturbed disk galaxy, with no major ongoing merging or other significant disruptive interactions.
