The galaxy presents an elongated morphology, with an apparent major axis likely exceeding twice the minor axis. The core region exhibits a concentration of light, appearing relatively bright and somewhat compact. It displays a yellow-orange hue, potentially indicative of an older stellar population, or a high degree of dust extinction. 

Moving outward from the core, the galaxy's light profile diminishes, displaying a fading disk-like structure. There are subtle hints of asymmetry in the outer regions of the disk; these features could potentially be interpreted as signs of tidal disturbances. Overall, the galaxy appears relatively smooth, with no definitive spiral arm structure immediately obvious. 
