The observed galaxy presents a generally blue disk structure with notable spiral arms. The arms are well-defined and extend outwards from a moderately sized central bulge. The bulge appears to be yellowish, suggesting an older stellar population, while the spiral arms exhibit a bluer hue, indicative of ongoing star formation.

There is no obvious presence of a strong bar structure. The disk is not perfectly edge-on but appears at an oblique angle to the line of sight, allowing the spiral arm structure to be clearly observed. There is no obvious sign of any major merger events, but there seems to be minor disturbances in the symmetry of the spiral arms. The galaxy does not have a clearly smooth, elliptical morphology.
