This galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a strong concentration of light, appearing yellow-orange in color, suggesting an older stellar population. Moving outward from the core, the color profile shifts subtly toward a greenish hue. This suggests the presence of a younger stellar population that is bluer than the core stars. The overall shape approximates a flattened sphere. There is no apparent spiral arm structure or significant dust lane features visible. The galaxy does not display signs of any major ongoing merger activity or significant tidal disturbances in this image. However, there might be minor disturbances visible.
