The galaxy presents as a somewhat elliptical structure, with a pronounced central bulge. The core exhibits a high degree of luminosity, suggesting a concentration of older stars, possibly with a supermassive black hole actively accreting material at the center. The overall color is slightly redder compared to the outer regions, indicating an older stellar population or a higher dust content. The disk component appears relatively smooth, with only subtle indications of spiral arm structure. The galaxy's morphology suggests it is an early-type spiral galaxy.
