The galaxy appears to be a luminous, elliptical galaxy with a smooth, centrally concentrated light profile. Its shape is elongated with a high degree of symmetry. The core exhibits a bright, golden-yellow hue, suggesting a population of older stars. Fainter, greenish light extends outward from the center, possibly indicating the presence of some younger stellar populations or nebular emission. No distinct spiral arms or prominent dust lanes are visible. The overall structure suggests the galaxy is relatively undisturbed, showing no major signs of recent mergers or tidal interactions, although a possible minor asymmetry is suggested on the Northwest edge of the galaxy.
