The galaxy presents as a relatively smooth, elliptical structure. Its overall color profile indicates a dominance of older stellar populations, giving it a yellowish hue. There is a concentration of light towards the center, suggesting a prominent galactic nucleus or bulge. While it appears mostly round, there's a slight elongation. No prominent spiral arms or dust lanes are visible. There are signs of a possible interaction, with a disturbance above the galaxy, but it is difficult to determine if the interaction is currently happening, or if it is simply a superposition of a foreground object. There is no evidence of intense, recent star formation, but given its size, it is a massive galaxy.