The galaxy appears to be a spiral galaxy with a prominent, bright central bulge. The disk is visible, though not highly resolved, showing a slight inclination relative to our line of sight. Hints of spiral arms can be discerned, although they appear somewhat diffuse and not sharply defined, giving the galaxy a somewhat flocculent appearance. The galaxy's overall color is yellowish-white, suggesting a population of older stars, particularly in the bulge. There is some evidence of bluer regions within the disk, possibly indicating areas of more recent star formation, although these are not particularly prominent. The galaxy does not show any obvious signs of a major ongoing merger, though there could be some minor disturbances present within the spiral structure. The galaxy appears to be a relatively massive system, given the brightness of its bulge. Overall, it presents as an intermediate spiral galaxy, likely at a moderate redshift.
