The galaxy presents as a relatively compact and smooth object. Its morphology is primarily spheroidal, with a high degree of central concentration. The color gradient suggests an older stellar population dominating the core, trending towards redder hues. The outer regions exhibit a bluer tint, potentially indicating the presence of a younger, though still subdued, stellar population. There's no visible evidence of spiral arms, a distinct disk, or ongoing major mergers. Minor asymmetries are subtly present, indicating possible past interactions or minor disturbances. The overall structure appears settled, suggesting a system approaching quiescence in its evolutionary stage.
