The galaxy exhibits a disk-like morphology, though its orientation is not perfectly edge-on nor face-on. A prominent bulge is observed, occupying a considerable fraction of the galaxy's overall visual extent. Evidence of spiral arm structure is present, with the arms appearing somewhat loosely wound. There's possible distortion in the disk, indicating that the galaxy may have experienced past interaction, or perhaps is currently undergoing a minor merger with a smaller object. In terms of color, a relatively redder hue is evident in the central bulge, gradually shifting to bluer tones in the outer spiral arms.
