The galaxy presents as a well-defined spiral galaxy, inclined significantly relative to our line of sight. The bulge appears relatively small and concentrated, displaying a yellowish hue, which may indicate an older stellar population. Two distinct spiral arms are visible, emerging from the central bulge and extending outwards. These arms exhibit a somewhat flocculent structure, characterized by intermittent bright knots, possibly regions of active star formation. The arms show a relatively tightly wound morphology. There is no apparent evidence of a significant bar structure. The overall color of the galaxy is bluish-white in the disk, suggesting the presence of younger, hotter stars and ongoing star formation within the spiral arms. No obvious signs of a major merger event are apparent, though some minor irregularities in the arm structure may indicate some gravitational interactions. The overall smoothness of the galaxy's light profile suggests a late-type spiral classification.
