The galaxy presents a generally smooth morphology, appearing elliptical in shape. Its core exhibits a concentrated, bright golden-yellow hue, which gradually fades into a greenish halo. There's a slight elongation, but no signs of spiral arm structures or significant dust lanes are visible. The galaxy doesn't show signs of any major mergers or disturbances. It is a relatively isolated, well-defined structure. The color suggests older stellar populations are dominant, hinting at a relatively low star formation rate.
