The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, slightly off-white hue suggestive of a population of older stars. Extending outward from the central region is a fainter, diffuse halo or bulge. This outer region appears more reddish than the central core, possibly indicating a difference in stellar populations or dust content. There is a slight asymmetry to the galaxy's shape; it is mostly round, but not perfectly so. There are no obvious spiral arm structures or significant dust lanes visible within the galaxy's disk, although there is some hint of subtle disturbances. The galaxy doesn't show any obvious signs of a major ongoing merger event, but there appears to be a minor warp or slight asymmetry that may indicate a past interaction or minor disturbance.
