The galaxy presents as a relatively smooth, rounded structure with a concentrated central region. There's a slight elongation, but the overall shape leans towards circular. The color distribution indicates a population of older stars, primarily visible in the central bulge, with a bluer hue extending outwards, suggesting a small amount of ongoing star formation. The galaxy shows no signs of major disturbances or mergers in its current morphology, although a minor asymmetry could suggest a past interaction.
