The galaxy presents as a smooth, elliptical-like structure, with no apparent spiral arms or distinct disk features. The central bulge exhibits a concentrated, bright yellowish-white hue, suggesting a high density of older stellar populations. The isophotes appear largely regular, indicating a well-mixed and dynamically relaxed system. There is a slight elongation to the galaxy's overall shape, deviating marginally from perfect circularity. The faint outer regions display a gradual decrease in luminosity, fading into the background sky. Subtle color gradients are present, with the core exhibiting a somewhat bluer color, possibly due to a small amount of on-going star formation. No major signs of tidal disturbances or ongoing mergers are apparent in the morphology.
