The galaxy presents as a spiral type, observed at an angle somewhat inclined from face-on. A prominent central bulge is visible, exhibiting a bright, concentrated luminosity gradient that decreases outward. Spiral arms emanate from the bulge, displaying a moderately flocculent structure characterized by patchy regions of star formation indicated by the bluish color. These arms appear relatively tightly wound. There is a hint of dust lanes that follow the arms, which may be lightly obscuring and reddening the starlight. The overall shape appears elongated, suggesting a bar structure may be present, though it is not sharply defined. The light is distributed smoothly, without clear signs of ongoing major merging events. The color profile suggests the presence of a relatively old stellar population with a younger population scattered throughout the arms.
