The galaxy exhibits a clear spiral structure, with a central bulge that appears moderately sized. The spiral arms are relatively well-defined and are wound moderately tightly around the bulge. Evidence of a bar feature is present, appearing moderately strong and cutting through the central bulge region. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. There is some indication of ongoing star formation within the spiral arms, as suggested by the slightly bluer colors observed in those regions compared to the yellowish hue of the bulge. The galaxy is not viewed perfectly face-on, but at a slight angle. 
