The galaxy presents a generally smooth, elliptical morphology. The core exhibits a concentrated luminosity, appearing bright yellow. Moving outward, the galaxy transitions to a fainter and slightly bluer hue in its outer regions. The overall shape is largely round with a moderate degree of ellipticity, lacking any prominent spiral arms or distinct disk features. There's no obvious indication of any ongoing major merger events, though subtle asymmetries might suggest a minor interaction or disturbance in its recent history. The gradual color gradient from the core to the outer regions indicates a probable radial change in stellar populations. 
