The galaxy presents as a relatively smooth, elliptical structure. The core is a bright, concentrated region exhibiting a yellowish hue, suggestive of an older stellar population. Moving outward from the core, the galaxy displays a subtle color gradient, transitioning to a slightly bluer tone, implying the presence of a younger stellar population in the outer regions, but it's not particularly pronounced. There is a hint of a disk-like structure, though it lacks well-defined spiral arms or prominent dust lanes. There is a minor asymmetry present, indicating a possible past interaction or merger event. The overall morphology is consistent with an early-type galaxy undergoing some level of star formation.
