This galaxy presents as a generally smooth, elliptical morphology with a high degree of central concentration. The light distribution suggests a relatively old stellar population dominating the core, inferred from the yellowish hue. A slight flattening is observed, giving it a somewhat lenticular appearance. There is a hint of bluer light in the outer regions which may indicate ongoing star formation, though limited. No prominent spiral arms or dust lanes are discernible. The overall impression is that of a mature galaxy with a significant bulge component.
