The galaxy presents a somewhat flocculent spiral structure, though features appear partially obscured, likely due to distance. A moderately sized bulge dominates the central region, exhibiting a yellowish hue. Hints of spiral arms emerge from the core region, branching out into the galactic disk. A general blue-green tint pervades the spiral arms suggesting ongoing, though not particularly vigorous, star formation. The disk is oriented close to face-on relative to our line of sight. There is no obvious evidence of a strong bar structure present. The object exhibits signs of minor disturbances within the disk, suggesting the possibility of past or ongoing interactions, although no significant merger events are evident. The galaxy appears relatively smooth in its overall morphology, with a notable absence of large-scale irregularities.
