The galaxy presents as a centrally concentrated, smooth object. It exhibits an overall elliptical morphology, appearing nearly circular. The central region is noticeably brighter and has a yellow-white hue, suggesting an older stellar population. Moving outward from the core, the color shifts to a bluish tint, possibly indicating the presence of younger, hotter stars. The galaxy appears relatively undisturbed with no major signs of tidal features, strong spiral arms, or ongoing mergers. There may be minor irregularities in the outer regions that warrant further investigation.
