The galaxy presents as a spiral type, viewed at an inclined angle relative to our line of sight. The central bulge appears prominent and exhibits a yellowish hue, suggesting an older stellar population. The spiral arms are tightly wound and extend outwards from the bulge, displaying a bluish tint, indicative of ongoing star formation. Dust lanes appear to be present within the spiral arms, obscuring some of the starlight. There is a hint of a possible bar structure within the central region of the galaxy. The overall morphology suggests a relatively undisturbed galaxy, with no clear signs of a major ongoing merger, although some minor irregularities in the spiral arms cannot be ruled out. The disk of the galaxy appears to be more prominent than the bulge. There is a high degree of symmetry between the two sides of the galaxy.