The galaxy appears to be a spiral type, exhibiting a central bulge surrounded by a prominent, albeit somewhat diffuse, disk. There is evidence of spiral arm structure, although it is not sharply defined. A bar feature appears to bisect the central bulge, running along the main axis of the disk. The bulge appears moderate in size relative to the disk, and it presents a noticeable color gradient transitioning from a yellowish hue at the core to a more reddish tint towards its outer regions. The disk itself shows a mottled texture, indicating regions of varying stellar density or dust obscuration. No obvious signs of strong tidal interactions or recent major mergers are apparent; however, subtle irregularities in the disk might suggest minor disturbances. The galaxy is observed at a relatively high inclination angle, but not fully edge-on, allowing for a partial view of the spiral arm morphology.
