The galaxy presents a generally elliptical morphology, appearing as a smooth, concentrated spheroid of light. The central region exhibits a high degree of luminosity, suggesting a dense concentration of stars and potentially a supermassive black hole actively accreting matter. The galaxy appears nearly circular, with only a subtle elongation. The overall color is slightly red, indicating an older stellar population with relatively little ongoing star formation. There is no readily apparent disk structure or spiral arm features.
