The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region appears bright and slightly yellow. A faint, diffuse halo surrounds the central bulge, fading into the background sky. There is no clear evidence of spiral arms or a prominent disk structure. The overall color suggests a population of older stars, with minimal dust obscuration. There appears to be no major disturbance visible, such as tidal tails or obvious signs of an ongoing merger.
