The galaxy presents as a relatively smooth, elliptical morphology. Its light profile appears centrally concentrated, with a core region exhibiting a brighter, possibly yellowish hue, suggesting an older stellar population or dust obscuration within. Moving outward from the core, the color becomes slightly bluer. The radial light distribution appears fairly regular, with a gradual decrease in intensity moving away from the center. No distinct spiral arm structures or bar features are apparent in the image. The overall shape seems close to round, though there may be a slight elongation along one axis. There's no obvious indication of any major ongoing merger activity or strong tidal disturbances. There is a possibility of minor disturbances, but difficult to observe from this image.
