This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that transitions into a more diffuse halo. The core displays a yellowish-white hue, suggesting a population of older stars. The outer regions of the galaxy are fainter and exhibit a slightly bluer color, potentially indicating the presence of some younger stars or ongoing, though modest, star formation. No distinct spiral arms or prominent dust lanes are visible in this image. The overall morphology suggests a well-evolved system, likely with a significant stellar mass. Based on its smoothness, roundness, and lack of apparent merging activity, this galaxy appears undisturbed and relatively isolated.
