The galaxy presents as a centrally concentrated object with a largely smooth morphology. There appears to be a slight ellipticity to the overall shape. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Fainter, diffuse light extends outwards from the core, transitioning to a more reddish and slightly greenish color in the outer regions. The smoother distribution of light indicates a potential lack of prominent spiral arms or other distinct structural features. There is no noticeable presence of tidal tails or other strong signs of recent or ongoing major mergers. The galaxy appears relatively undisturbed.
