The galaxy presents as a disk galaxy, though is presented at a moderate inclination, not quite edge-on. The central bulge exhibits a smooth, concentrated appearance, suggestive of an older stellar population. The disk shows some faint structure and a mottled texture, indicating the presence of star formation regions, though not highly pronounced. There are areas of blue hue within the disk, which may correspond to young stars. Dust lanes are either absent or not clearly resolved. The galaxy appears relatively isolated, with no immediately apparent tidal features or companion galaxies indicating recent major merger activity. The galaxy's morphology leans toward a quiescent state with moderate disk activity.
