The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on from our vantage point. A central bulge is visible, appearing relatively smooth and concentrated, with a yellowish-orange hue, indicating a potentially older stellar population. Extending outwards from the bulge, the galactic disk exhibits a bluer tint, possibly indicative of younger, hotter stars. Some regions within the disk appear slightly mottled, suggesting the presence of dust lanes or star-forming regions, though these features are not highly prominent. Overall, the galaxy appears to be undergoing minimal major merging or disturbances, with a generally regular morphology. Evidence suggests a prominent, fairly flat disk with a slight warping visible at the lower edge.
