The galaxy presents a largely smooth, elliptical morphology. It appears moderately concentrated with a centrally bright core that emits strongly at redder wavelengths, suggesting an older stellar population. A very slight disky component cannot be ruled out, but any spiral structure is not readily apparent. The galaxy exhibits a fairly high degree of roundness, with only minor deviations from a perfect circle. There is no obvious evidence of major mergers or significant tidal disturbances. Overall, the galaxy’s light distribution suggests a well-evolved system with relatively low current star formation activity.
