The galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated bulge with a yellowish-orange hue, suggesting a population of older stars. Moving outwards from the center, the light gradually fades into a more diffuse halo. Hints of blueish color in the outer regions suggests the presence of a younger, star-forming stellar population. The overall morphology suggests a system that has largely undergone the process of morphological quenching, resulting in reduced star formation activity within the main body. There are no obvious signs of significant tidal disturbances or ongoing major mergers, indicating it is in a relatively relaxed state. The galaxy's light profile appears relatively smooth, with only subtle deviations from a perfect ellipse.
