The galaxy presents as a spiral galaxy with a substantial disk component. Its orientation is oblique to our line of sight, providing a somewhat face-on view that reveals discernible spiral arm structure. Two main arms can be seen winding loosely around the galactic center. The arms exhibit regions of bluish coloration, suggestive of ongoing star formation. The central bulge appears moderate in size and has a yellowish or whitish hue, indicating a population of older stars. Some degree of asymmetry or perturbation is evident, possibly suggesting minor disturbances or interactions. The disk is more elongated than circular. There is a slight suggestion of a bar-like structure in the center of the galaxy. The galaxy is actively forming stars at a moderate rate.
