The galaxy presents a largely smooth morphology, with a high degree of circularity. There's a distinct central bulge exhibiting a yellow-orange hue, which could indicate an older stellar population. The outer regions of the galaxy display a gradual decline in surface brightness. There's a very slight hint of a disk-like structure, but overall the galaxy appears predominantly spheroidal. No obvious signs of active star formation are immediately apparent in the image based on color. No tidal tails or distortions suggesting ongoing mergers are observed, implying the galaxy is relatively undisturbed.
