The galaxy presents as a disk-shaped structure, viewed at a moderate inclination. A prominent central bulge exhibits a concentrated, bright core, likely indicative of a high stellar density. The disk component displays spiral arm structures, albeit somewhat flocculent and patchy. Blue hues are visible within the spiral arms, suggesting regions of active star formation. Evidence of dust lanes are visible, particularly along the near side of the disk, obscuring some of the starlight. Faint tidal tails or disrupted features appear to extend outwards from the main body of the galaxy, primarily on the left side, suggestive of a possible past interaction or merger event. Overall, the galaxy appears to be in a state of moderate morphological disturbance.
