The galaxy presents as a predominantly blue-hued spiral structure, though the arms are somewhat indistinct and ill-defined, lacking sharp boundaries. There is a suggestion of a faint ring-like structure encompassing the main body, with a slightly greenish tint towards the outer edge. The core region appears relatively smooth, indicating an older stellar population with potentially reduced star formation. Irregular clumps and patches are distributed throughout the disk, suggestive of localized star formation regions. While not clearly defined, there is a subtle indication of ongoing tidal interaction, though strong merging features are absent. The overall morphology suggests a galaxy undergoing a period of minor disturbance, potentially from a past interaction that is now mostly quiescent.
