The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually fades into an extended, diffuse halo. The color profile shows a yellowish hue in the core, suggesting an older stellar population, with a slight bluer tint in the outer regions, possibly indicating the presence of younger stars. There is no discernible spiral arm structure. No significant tidal disturbances or obvious signs of recent merging events are apparent.
