The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge, transitioning outward to a less defined halo. The dominant color is a warm yellow-orange, suggesting an older stellar population and lower rates of ongoing star formation. There are some hints of bluer colors present, which would indicate the presence of some younger, hotter stars. Overall, the object appears relatively undisturbed, with no obvious signs of major mergers or tidal disruptions. 
