The galaxy presents a disk morphology, oriented approximately face-on relative to our line of sight. Spiral arm structures are faintly visible, emanating from a central bulge region. The bulge appears moderate in size relative to the overall galaxy. The spiral arms display some degree of patchiness, suggesting ongoing star formation regions within. The disk exhibits a blue hue, indicative of a younger stellar population, while the central bulge appears slightly redder, implying the presence of older stars. There appears to be a subtle asymmetry or minor disturbance in the disk morphology.
