The galaxy presents as an edge-on spiral, exhibiting a clear disk structure. A prominent central bulge is observed, displaying a concentrated, yellowish-orange hue, which may indicate an older stellar population. The disk component appears relatively smooth, with a bluer color gradient extending from the central bulge outwards, suggesting the presence of ongoing star formation. The galaxy appears slightly asymmetrical, possibly indicating minor gravitational interaction. Dust lanes within the disk are subtle but visible, contributing to the slightly mottled appearance. No major disturbances or signs of ongoing major merger events are immediately apparent.
