The galaxy presents a relatively face-on orientation. The central bulge appears moderately prominent. A disk is clearly visible, exhibiting spiral arm structures that are somewhat patchy. The arms are not very tightly wound, and their definition varies across the galaxy's face. There is a suggestion of a bar feature, but it is not distinctly prominent. Color variation is present across the galaxy; the central bulge displays a yellowish hue, possibly indicating an older stellar population, while the spiral arms show bluer colors, potentially indicative of ongoing star formation. Irregularities are visible in the disk, possibly due to minor disturbances or ongoing mergers with other objects.
