The galaxy presents as a moderately luminous object, with a smooth, elliptical morphology. There is evidence of an intermediate degree of central concentration, with a bright, yellowish core that gradually fades into a bluer, diffuse outer region. The galaxy exhibits a slight elongation, with a shape that appears to be somewhere in between round and cigar shaped. There are some minor disturbances that could indicate a past interaction with a small galaxy. There is no dust lane clearly apparent, nor is there evidence of strong spiral arm structure. The overall color suggests a mix of stellar populations, with older stars dominating the core and younger stars contributing to the bluer, less concentrated regions.