The galaxy presents as a slightly elongated, diffuse structure with a smooth overall appearance. It exhibits a dominant reddish-orange hue across its body, possibly indicative of an older stellar population and/or significant dust obscuration. There is a hint of greenish-blue color in its edges, suggesting a low level of on-going star formation within the galaxy, though this is a minor feature. The galaxy’s morphology appears relatively undisturbed with no clear signs of spiral arms or a prominent central bulge, and only slight indications of tidal features or distortions that would suggest a recent merger event. It possesses a considerable mass and high luminosity. 
