The galaxy presents as a relatively smooth, elliptical structure. Its light profile appears centrally concentrated, with a gradual decrease in brightness towards the outer regions. There is little to no evidence of spiral arms or a distinct disk component. The galaxy exhibits a subtle color gradient, with the core appearing slightly more red/yellow compared to the outer regions which have a blueish-white hue. This color variation could indicate differences in stellar populations, with potentially older, redder stars concentrated towards the center and younger, bluer stars in the periphery. There are no obvious signs of recent major merger activity or significant tidal disturbances. The overall morphology suggests a mature galaxy, likely an early-type system, with a predominantly old stellar population and a relatively low star formation rate.
