The galaxy appears to be an elliptical galaxy, characterized by its smooth, largely featureless morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the galaxy's core. The color gradient suggests that the central region is yellower, possibly indicating an older stellar population with fewer young, massive stars. The outer regions exhibit a bluer hue, hinting at the presence of a younger stellar population, or the influence of recent star formation, though it is still largely smooth. No significant tidal features or distortions are apparent, suggesting that the galaxy has not undergone any recent major mergers. It appears generally round with a small deviation toward an in between shape. Any substructure within the galaxy is subtle and difficult to discern at this resolution. The lack of distinct spiral arms or a prominent disk further supports the classification as an elliptical galaxy.
