The galaxy presents a distinct spiral structure. The arms are tightly wound and emanate from a central bulge that appears to be of moderate size. The disk is viewed at a slight angle, suggesting it is not perfectly face-on but is also not edge-on. The galaxy exhibits evidence of a bar structure spanning across the bulge area. The light distribution suggests a relatively smooth appearance overall, although the spiral arms are clearly discernible. No significant signs of major disturbances or merging activity are readily apparent in the galaxy's morphology, though there may be minor disturbances. The overall color suggests a mix of stellar populations, with a yellowish central bulge and bluer spiral arms, possibly indicative of active star formation within those regions.
