The galaxy presents a predominantly smooth morphology, exhibiting a central bulge that gradually fades into its outer regions. It appears to be an elliptical galaxy. The color profile is relatively uniform across the galaxy, with a slight tendency towards redder hues, indicating an older stellar population and a decreased rate of star formation. There is no obvious spiral structure or dust lane. The galaxy is somewhat round, showing a high concentration of luminosity towards the center. There are no obvious signs of ongoing merger activity or significant tidal disturbances.
