The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is largely round, with no apparent disk or spiral arms. The light distribution is concentrated towards the center, indicating a substantial bulge component. There's a gradual decrease in luminosity from the core to the outer regions, and the color suggests an older stellar population, potentially with a lower rate of ongoing star formation. Faint color variations hint at underlying features, though the resolution limits detailed characterization. No significant signs of tidal disturbances or ongoing mergers are readily apparent. The overall morphology suggests a galaxy that is evolved and quiescent.
