The galaxy presents as a spiral galaxy with a notable central bulge, likely hosting a supermassive black hole at its core. The arms are prominent, tightly wound around the central bulge. There appears to be a moderate amount of recent star formation occurring within the arms as suggested by the presence of pockets of light. The galaxy exhibits a relatively smooth morphology, with no clear signs of major interaction or recent merging events with other galaxies. The disk component of the galaxy displays an inclination with a moderate amount of dust. The galaxy has a regular shape without any major distortion or tidal features. The structure exhibits indications of a bar feature, likely contributing to gas inflow towards the central region. The spiral arms show a two-armed structure, with some winding.
