The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core region exhibits a yellowish-orange hue, suggesting an older stellar population. Moving outwards from the core, a gradual transition to a bluer color is observed, possibly indicating the presence of younger stars or ongoing star formation in the outer regions. The overall shape appears predominantly round, showing minimal signs of significant distortions or tidal features. There is a subtle suggestion of a disk-like structure, although this is not definitively confirmed in the image. There are no signs of an ongoing or recent major merger, although the potential for minor disturbances cannot be ruled out.
