The galaxy presents as a relatively smooth, lenticular or early-type spiral system. It exhibits a bright, concentrated central bulge that appears yellowish.  The surrounding disk component is less luminous, with a bluish tinge, suggesting the presence of younger stellar populations and ongoing star formation, albeit at a moderate level.  The disk appears somewhat elongated, deviating from perfect circularity; however, no strong tidal features or distortions are evident, indicating that the galaxy is likely not undergoing a major merger event, although minor disturbances cannot be ruled out.  The overall structure suggests a relatively evolved galaxy, possibly transitioning from a spiral-dominated morphology toward a more elliptical form. The luminosity profile implies a considerable stellar mass.  The lack of pronounced spiral arms or prominent dust lanes further supports the classification as a smooth disk galaxy.