The galaxy presents a relatively smooth, elliptical morphology, characterized by a high degree of central concentration. The light distribution suggests a spheroidal structure, with a gradual decrease in surface brightness from the core outwards. There is no distinct spiral arm structure visible, or any significant dust lane features. The galaxy's color appears slightly redder, possibly indicating an older stellar population and lower star formation rate. The galaxy exhibits an overall elliptical shape with slight elongation. There is no evidence of a major ongoing merger or significant tidal disturbances based on the image. The general shape appears to be relatively smooth and undisturbed.
