The galaxy presents as a smooth, elliptical-like structure with a highly concentrated central bulge. Its overall shape is noticeably rounded. The core exhibits a bright, yellowish hue, suggesting a population of older stars. Moving outward from the center, the color gradually shifts to a slightly redder tone. There are no prominent spiral arms or dust lanes visible; the light distribution appears relatively uniform. Based on the apparent color and morphology, this galaxy is likely a relatively massive system with a low star formation rate. No signs of significant tidal disturbances or ongoing merging events are apparent in the image.
