The galaxy presents as a relatively smooth, elliptical form. Its light profile exhibits a centrally concentrated structure with a gradual falloff in intensity towards the outer regions. The central region appears to be dominated by older stellar populations, indicated by its yellowish-red color. The outer regions show a bluer tinge, suggesting the presence of some younger, hotter stars, but the overall color profile indicates a largely quiescent system. There is no clear evidence of spiral arms, a disk structure, or significant dust lanes. The galaxy appears undisturbed, lacking any obvious signs of ongoing mergers or tidal interactions with other galaxies. The ellipticity suggests a non-negligible angular momentum, though it is still predominantly dispersion-supported rather than rotation-supported. Overall, it has a smooth, elliptical morphology.
