The galaxy presents as a spiral galaxy with a moderate inclination relative to our line of sight. Its morphology reveals a prominent central bulge, exhibiting a yellowish-white hue, indicative of an older stellar population. The spiral arms are clearly defined, demonstrating a multi-armed structure. The arms are wound relatively tightly around the bulge. These arms display a bluer color, suggesting ongoing star formation. There appears to be a weak bar structure present across the bulge. No significant tidal features or signs of a major merger event are immediately apparent, although minor disturbances cannot be ruled out.
