The galaxy presents as a relatively smooth, concentrated object with an overall elliptical morphology, indicating a spheroid-dominated system. Its color appears predominantly reddish-yellow, suggesting an older stellar population with lower ongoing star formation. The light distribution is highly centralized, with the brightest region concentrated in the galaxy's core, although there is a subtle double nuclei that could be a tidal effect or minor merger. There does not seem to be any indications of strong spiral arm structures. The object appears undisturbed, lacking any signs of tidal tails or other major morphological distortions.
