The galaxy presents as a centrally concentrated, elliptical-like object. A bright, relatively smooth central bulge dominates the overall structure, exhibiting a yellow-orange color. There is a subtle transition towards a less concentrated, fainter, and bluer region extending outwards from the bulge, which suggests the presence of a disk component. No prominent spiral arms are discernible, and the overall light distribution appears relatively uniform within the observed disk. There is no evidence of major tidal features or obvious signs of an ongoing merger. The morphology suggests this is a massive galaxy that is currently not forming many new stars. 
