The galaxy appears to be a spiral galaxy, viewed approximately face-on. It exhibits well-defined spiral arms which show a winding structure that appears to be of medium tightness. The nucleus presents a yellow hue, suggesting a population of older stars, and a possible central bulge. Blue regions are observed within the spiral arms, indicating areas of active star formation, and it suggests the presence of younger, hotter stars in these areas. There's some indication of flocculent structure within the arms. A faint bar is either weak or absent, and the size of the bulge is relatively small. There are no obvious signs of major tidal disruption or recent major merger events.
