The galaxy presents a disk-like morphology, observed at a significant inclination relative to our line of sight. Two prominent spiral arms are observed emanating from a central bulge. The spiral arms display a moderate degree of winding. The central bulge appears yellow-white in color. The overall structure exhibits a relatively smooth appearance, with no apparent signs of major mergers or significant tidal disturbances. A bar structure appears present. The blueish color suggests a moderate presence of younger stellar populations and ongoing star formation.
