The galaxy exhibits a generally smooth morphology, with a dominant spheroid component. The light profile suggests a concentrated nucleus with a gradual decrease in intensity outward. The galaxy displays an elliptical shape, appearing nearly round but slightly elongated. There is no apparent spiral arm structure or significant dust lane obscuration visible in this image. A subtle color gradient is observed, with a more yellowish hue toward the core and a bluer tint in the outer regions, potentially indicating differences in stellar populations or dust content. No signs of significant tidal disturbances, major mergers, or interacting companions are discernible.
