The galaxy presents as a disk galaxy, observed nearly edge-on. A prominent central bulge dominates the core, exhibiting a smooth, rounded morphology. The disk appears relatively thin and extended, with a slight warp noticeable. Dust lanes are faintly visible along the plane of the disk, causing some obscuration of starlight. The overall color profile suggests an older stellar population, although hints of bluer regions may indicate localized areas of recent or ongoing star formation. There appears to be no strong evidence of tidal disturbances or ongoing merger activity.
