The galaxy presents as a spiral galaxy, observed at an inclination that is neither face-on nor edge-on, but rather at an intermediate angle. This angle allows for some, albeit blurred, structural features to be visible. The central bulge appears bright and concentrated, with a yellowish hue, suggesting an older stellar population. Diffuse spiral arms extend outward from the bulge, exhibiting a bluer color, indicative of more recent star formation activity. The arms are somewhat tightly wound. There is faint evidence of a bar structure that runs through the bulge. The galaxy's disk is well-defined. The galaxy does not appear to be undergoing any major mergers, however, there may be some minor disturbances in the shape of the spiral arms, especially in the outer disk.
