The galaxy exhibits a prominent, centralized bulge with a yellowish hue, indicating a concentration of older stars. The disk is clearly visible, displaying a distinct spiral structure. Two primary spiral arms appear to emanate from the central bulge, with hints of branching or additional arm segments visible. These arms show a moderately tight winding pattern. The overall color gradient suggests that the galaxy has ongoing star formation, particularly within the spiral arms where bluer regions are observed. There is no obvious indication of major merging or significant tidal disruption. Faint dust lanes may be present within the spiral arms, but this is difficult to determine definitively given the image resolution. The galaxy appears relatively face-on, providing a clear view of its disk and spiral structure.
