The galaxy appears to be a relatively smooth, elliptical galaxy with a dominant central bulge. It exhibits a spheroidal morphology with a high degree of circularity. The light profile appears concentrated toward the center, suggesting an older stellar population. Some faint extended structure is observed surrounding the main body of the galaxy. No distinct spiral arm features are apparent. The color is slightly reddish, indicating a population of evolved stars with little ongoing star formation. There is no evidence of tidal tails or major disturbances, but some irregularity around the perimeter of the galaxy may indicate a minor interaction or past merger event.