The galaxy presents as a spiral galaxy, viewed at an angle that is slightly off from being face-on. The spiral arms are well-defined, exhibiting a relatively high degree of symmetry. Two arms are clearly visible, and their winding is of medium tightness. There is evidence of flocculent structure within the spiral arms, suggesting ongoing star formation. The arms display varying color intensities. The central bulge region appears relatively small and subdued. Within the center is a bright region, likely around a supermassive black hole. There are a few blue areas within the arms, which also suggests star formation. There appears to be a faint bar structure that is oriented along the center. Overall, the galaxy appears relatively undisturbed, with no obvious signs of any major recent mergers or tidal interactions.
