The galaxy presents as a spiral galaxy, observed at an oblique angle, inclined relative to our line of sight. It has a prominent central bulge that appears relatively smooth and concentrated. The spiral arms are visible, although not sharply defined, suggesting they are somewhat diffuse or loosely wound.

There is evidence of dust lanes within the spiral arms, indicated by darker, less luminous regions that obscure the starlight. The overall color of the galaxy suggests a mix of stellar populations, with some bluer regions indicating ongoing star formation and redder regions populated by older stars. The galaxy does not appear to be strongly interacting or undergoing a major merger.
