The galaxy presents a somewhat inclined disk morphology. A central bulge is discernible, appearing moderately bright and concentrated. Faint spiral arm structures emanate from the central region, extending into the outer disk. The arms appear flocculent, with regions of enhanced star formation indicated by a bluer color, especially in one of the arms. The disk exhibits a generally smooth appearance, with some irregularity in the arm structure. There is the suggestion of a bar feature crossing the central bulge, although this is not well-defined. The galaxy appears to be undergoing relatively active star formation, particularly within the spiral arms. The overall color is intermediate, suggesting a mix of stellar populations. There is some asymmetry present in the galaxy's structure.
