The galaxy presents as a spiral type, exhibiting a discernible disk structure. Spiral arms are present, but their morphology is somewhat disrupted. There are indications that the galaxy is currently undergoing a merger or experiencing tidal interactions, with asymmetry observed in the distribution of its light and stellar components. The arms appear tightly wound in some regions and looser in others.

A central bulge is present and moderately sized. Evidence of a bar structure is suggestive, but not definitively conclusive. The galaxy has a bright, central region, possibly indicating an active galactic nucleus or a high concentration of stars in the core. The galaxy demonstrates a blueish hue in the arms, suggesting that the disk is active in star formation. 
