This galaxy appears to be relatively compact. It exhibits a dominant, smooth central bulge with a slightly elliptical, though largely rounded, morphology. There is a hint of disturbed structure or a minor interaction occurring within the central region, as evidenced by some asymmetric light distribution. This is further supported by the faint tidal features around the galaxy that hint at past interaction or merger activity, potentially indicating a merging system that is either faint or hard to resolve. The color gradient within the galaxy suggests the presence of varying stellar populations. The inner regions appear to exhibit bluer colors, possibly due to recent star formation. Overall, the galaxy appears to be a potentially disturbed system with a mostly smooth morphology. 
