The galaxy presents an elliptical morphology, exhibiting a smooth, centralized concentration of light. The core region displays a yellowish-orange hue, suggesting a population of older stars. Moving outwards from the core, the galaxy's color gradually shifts towards a slightly bluer tone in the outer regions. This could indicate some ongoing, albeit weak, star formation in these areas. No distinct spiral arm structures are discernible. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal distortions. It maintains a generally round appearance, with a slight deviation towards a more elongated shape. Overall, the galaxy appears to be a relatively massive system with characteristics of a quiescent elliptical galaxy undergoing minimal current star formation activity.
