The galaxy presents as an edge-on spiral or lenticular system. A prominent central bulge is visible, displaying a slightly oblate, rounded morphology. The disk is observed at a nearly perpendicular angle to our line of sight. Evidence suggests dust lane obscuration along the galactic plane, contributing to a reduction in flux emanating from the central regions and providing contrast along the disk. The overall color suggests a significant population of older stars, particularly within the bulge. Hints of bluer star formation regions are visible, possibly indicating more recent, though potentially localized, star formation activity. The smooth appearance, combined with its high degree of disk inclination, may indicate a more evolved system where spiral arms, if present, are tightly wound or diffuse. There does not appear to be any signs of strong tidal interactions or ongoing major mergers.
