The galaxy presents a largely smooth, elliptical morphology. Its core appears bright and concentrated, exhibiting a yellowish hue, suggesting an older stellar population. Surrounding the central region, the galaxy gradually diffuses outward, maintaining a generally elliptical shape.  There is a slight asymmetry in the light distribution with a faint reddish patch observed on one side of the core, possibly indicating an area of ongoing or recent star formation activity. The outer regions fade into the background sky, indicative of a decreasing stellar density with increasing distance from the galactic center. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
