The galaxy displays a distinct spiral morphology, though it is presented at a near edge-on inclination. Two tightly wound spiral arms are observed emanating from a central bulge region. The bulge itself appears relatively small in comparison to the overall disk size. There is no obvious presence of a strong bar structure bisecting the bulge. Minor disturbances are visible in the outer arms, potentially hinting at past or ongoing interactions. The spiral arms exhibit a bluish hue, suggestive of ongoing star formation.
