The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central region, suggesting a possible bulge component. The overall color profile seems redder, which might indicate an older stellar population. There's a lack of discernible spiral arms or significant dust lanes, reinforcing the impression of a galaxy nearing the end of its star formation period. The object's overall shape appears somewhat rounded, and does not suggest any signs of merging events or major disturbances. Based on the colors, luminosity, and overall morphology, this galaxy is most likely a massive elliptical galaxy with a low star formation rate.
