This galaxy exhibits an overall elliptical morphology, with a noticeable bulge at its center. The central region appears to be populated by older stars, indicated by its yellowish-orange hue. Moving outwards from the center, the color transitions to a more blueish-white, suggesting the presence of younger, hotter stars in a disk-like structure. However, this disk is not sharply defined. The galaxy appears relatively smooth in texture, but there are some subtle indications of minor disturbances or asymmetrical features in the outer regions, possibly resulting from past interactions or mergers. These features are not prominent, implying that if a merger event occurred, it was likely minor and occurred in the distant past. There may be limited on-going star formation, mainly located in the disk. 
