The galaxy presents a largely smooth, elliptical morphology. Its central region exhibits a high degree of luminosity, concentrated in a roughly circular area. Progressing outward, the galaxy’s luminosity gradually diminishes. While a distinct spiral arm structure is not evident, the galaxy is not perfectly spherical, displaying a slight elongation. There are no obvious signs of tidal disturbances or ongoing mergers. The core color appears shifted towards redder wavelengths. Based on the observed characteristics, the galaxy likely has a substantial mass and a moderate rate of star formation.
