The galaxy presents as a relatively small, highly flattened disk galaxy, viewed nearly edge-on. It exhibits a prominent central bulge that appears smooth and concentrated. The disk is thin and shows limited evidence of spiral arm structure or star-forming regions. The light distribution suggests an older stellar population, with a lack of bright, blue star formation. Faint hints of dust lanes are visible within the disk, near the central bulge, indicating the presence of interstellar material. The overall appearance points toward a system that is evolving towards a more passive state, with a reduced rate of star formation. There is no significant morphological disturbance evident, indicating that it has not experienced a major merger event recently.