The galaxy presents as a luminous, elliptical structure. The central region exhibits a high degree of smoothness, with a gradual decrease in luminosity observed towards the outer edges. The galaxy appears predominantly smooth, with no obvious spiral arm structures or significant dust lanes visible. There is a slight elongation, deviating minimally from a perfectly circular morphology. The galaxy's color profile suggests a population of older stars. The overall light distribution implies a relatively quiescent system, lacking prominent features indicative of recent major merger events or strong star formation. Slight indications of minor disturbances may be present.