The galaxy presents as a relatively well-defined, disk-shaped system, observed edge-on from our vantage point. A prominent central bulge, exhibiting a yellowish hue, dominates the galaxy's core, suggesting a concentration of older stellar populations. The disk component, extending outwards from the bulge, appears flattened and elongated, with a bluer color gradient towards the edges, indicative of ongoing or recent star formation. Faint dust lanes are suspected near the disk midplane, but resolution limits conclusive confirmation. Overall, the galaxy exhibits a smooth, largely undisturbed morphology.
