The galaxy presents as a generally smooth, elliptical-like structure. The galaxy exhibits a concentrated, bright core that fades outward into a more diffuse halo. The central region shows a bluer hue, suggesting the presence of younger, hotter stars. The galaxy appears to be fairly isolated, with no obvious signs of major mergers or significant tidal disturbances, though there are some hints of minor perturbations in the overall shape. The morphology is largely smooth, consistent with an early-type galaxy that has largely completed its star formation. There is no prominent disk structure. Based on the colors, this galaxy is potentially undergoing relatively modest star formation. The overall shape appears somewhat elongated, but not strongly cigar-shaped.
