The galaxy exhibits a distinct spiral structure, characterized by prominent, well-defined arms. Two arms are clearly discernible, originating from a central bulge region. The arms display a moderate winding, neither tightly coiled nor loosely extended. The arms themselves appear somewhat patchy, with varying brightness along their length. This could suggest differing stellar densities or active star formation regions within the arms.

The central bulge appears moderate in size relative to the overall galaxy diameter, displaying a smooth texture with a yellow hue. There's a subtle elongation of the galaxy disk, indicating a departure from a perfectly circular profile. The overall color profile suggests a mix of stellar populations, with bluer regions within the spiral arms possibly indicating younger stars and reddish-yellow hues in the bulge suggesting older, redder stellar populations. The structure presents indications of disturbances, which could suggest the galaxy has experienced recent interactions or a minor merger event.
