This galaxy exhibits a somewhat elongated, disk-like morphology. The central region displays a bright, concentrated bulge, suggesting a relatively high stellar density. The disk component appears inclined relative to our line of sight, presenting an almost edge-on orientation. Dust lanes are faintly visible within the disk, particularly along the edges, obscuring the starlight. Patches of bluer light, suggestive of younger stellar populations or star-forming regions, are distributed throughout the disk, but are concentrated mostly near the central bulge. There are also indications of faint tidal features or distortions, though these are not prominent. The overall structure suggests a spiral galaxy, potentially undergoing minor interactions or disturbances.
