The observed galaxy presents as a disk galaxy, viewed almost perfectly edge-on. It exhibits a significant central bulge which appears largely featureless and smooth, possessing a distinctly rounded shape. This bulge dominates the visual appearance of the galaxy. A faint, elongated disk is visible extending beyond the central bulge, bisecting the galaxy horizontally. There are minimal signs of recent mergers or tidal disturbances. The overall morphology suggests a relatively stable and mature system. The galaxy is luminous, particularly at its core, indicating a significant concentration of stars and potentially a central supermassive black hole actively accreting material.
