The galaxy appears as a somewhat flattened, elliptical structure with a smooth, centrally concentrated light profile. The core exhibits a yellowish-white hue, potentially indicating an older stellar population. The outer regions of the galaxy fade gradually into the background, displaying a slightly redder tint which could be attributed to a greater proportion of older, redder stars or dust obscuration. No distinct spiral arms or prominent dust lanes are discernible in this image. The overall morphology suggests the galaxy is relatively evolved and not undergoing significant recent star formation. There is no clear evidence of interaction with other galaxies, though subtle asymmetries could hint at minor disturbances.
