The galaxy presents as a centrally concentrated, relatively smooth object with an overall elliptical morphology. There is a subtle color gradient, with the core appearing slightly more yellow/gold in color compared to the outer regions. The outer regions fade gradually into the background, suggesting a lack of sharp edges or distinct spiral arm structures. There is a faint, extended halo visible, which might be composed of older stars. No significant tidal features or ongoing mergers are apparent. The galaxy's light distribution suggests a system dominated by an older stellar population with subdued star formation activity.
