The galaxy presents as a centrally concentrated system with a spheroid morphology. The core region exhibits high luminosity, suggesting a concentration of older stellar populations. The light becomes more diffuse towards the outer edges, which are still fairly circular. Faint dusty regions could exist but are difficult to see at this resolution. There is no strong evidence of spiral arm structure or a prominent disk. The overall color is yellowish-white, indicating a lack of significant ongoing star formation. The galaxy appears relatively undisturbed, showing no obvious signs of recent mergers or tidal interactions.
