The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge exhibiting a yellow-orange hue, indicative of an older stellar population. The outer regions display a subtle fading in intensity with no prominent spiral arm structures. The galaxy appears to be relatively undisturbed, showing no signs of major mergers or tidal disruptions. There are no significant dust lanes or prominent star-forming regions visible within the observed light. The object appears as a fairly well-defined, round structure. Based on the apparent color profile, the galaxy is likely at a significant cosmological distance. 
