The galaxy appears to be an elliptical galaxy, with a smooth, relatively featureless structure. Its light profile is concentrated towards the center, with a bright core that fades into a diffuse halo. There is a subtle color gradient, with the central region exhibiting a yellowish or slightly redder hue, and the outer regions appearing bluer. This suggests a population of older, redder stars in the core, potentially with some recent, low-level star formation in the outskirts. The galaxy's overall shape is close to round, with no obvious signs of a disk-like structure or significant tidal disturbances. The absence of prominent spiral arms or dust lanes further supports its classification as an elliptical galaxy. Overall, the morphology points toward a galaxy with a stellar mass likely above average, and a relatively low star formation rate at the time the image was taken.
