The galaxy presents as a centrally concentrated, relatively symmetrical object. Its light profile appears smooth with no obvious spiral arm structures or distinct morphological features such as bars. The color index suggests a relatively old stellar population, with a reddish overall hue, but with a slight blue shift in the very center. The galaxy appears largely undisturbed, showing no major signs of tidal interactions or ongoing mergers. Its shape is roughly circular. There may be a minor asymmetry in its outer regions, possibly suggesting a subtle interaction or past merger event, although this is difficult to confirm given the resolution.
