The galaxy presents as a spiral type with a moderately inclined disk. The central bulge exhibits a prominent, bright, yellowish-white hue, suggesting an older stellar population. The spiral arms are not tightly wound, indicating possibly an intermediate stage. Patches of blue light, indicative of younger, hotter stars, are visible within the arms, suggesting ongoing star formation. There appears to be some asymmetry in the arm structure, possibly indicating a past interaction or disturbance. The disk's surface brightness declines gradually away from the bulge. The overall shape is elongated, suggesting that this is not a face-on galaxy.
