The galaxy presents as a moderately bright, relatively compact object. Its light profile appears smooth and elliptical, suggesting a classification as an elliptical galaxy. The core exhibits a slightly more concentrated luminosity. There is a subtle color gradient, with the central region tending towards yellow-green. Given the apparent lack of distinct spiral arms or prominent dust lanes, the galaxy appears to be relatively evolved. Some minor distortions are apparent. Further spectral analysis would be valuable for more definitive determination of stellar populations and any active galactic nucleus within this galaxy.
