The galaxy presents an elliptical morphology, appearing largely smooth in structure with a high degree of central concentration. The color gradient shifts from a predominantly red core, suggestive of an older stellar population, to a greenish-yellow outer halo. This suggests the presence of a younger, bluer population of stars in the galaxy's periphery, though the color is fairly subtle. No obvious spiral arms or distinct dust lanes are discernible. There are no strong indications of any tidal features or significant ongoing merger activity. The overall appearance indicates that the system is relatively undisturbed.
