The galaxy exhibits a generally smooth morphology, with an elliptical shape. The central region presents a bright, concentrated core that appears yellowish-white, suggesting a population of older stars. The outer regions display a more diffuse, bluish halo extending outwards. The bluer color may indicate some presence of younger stars in the disk. A slight elongation is noticeable, giving it a somewhat cigar-like appearance. There seems to be some minor disturbance, possibly due to an ongoing or past interaction, which is causing some irregularity in the shape. No prominent spiral arms or distinct dust lanes are visible. The overall impression is of an evolved galaxy, relatively massive, with a moderate degree of ongoing star formation.
