The galaxy appears to be a relatively smooth, elliptical system. Its light profile exhibits a central bulge that is bright and yellowish in color, suggesting a population of older stars. Moving outward from the core, there is a gradual decline in brightness with a more diffuse, bluish halo. There are no clear indications of spiral arms or a well-defined disk. The overall morphology suggests a system that is more evolved, with limited ongoing star formation as suggested by the colors and texture of the outer regions. There is a faint hint of disturbance to the structure, but it appears relatively minor.
