The galaxy presents as a largely smooth, elliptical structure, exhibiting a high degree of central concentration. The core region appears bright and yellow. The luminosity diminishes gradually outward from the core, with the outer regions displaying a slightly bluer tint. There is a very subtle hint of disturbance in the outskirts, suggesting a possible minor interaction or past merger event. The overall shape is predominantly round, with a very slight deviation toward a cigar shape. No distinct spiral arms or bar structures are discernible. The galaxy exhibits colours consistent with a stellar population that has a moderate amount of on-going star formation.
