This appears to be a spiral galaxy, exhibiting a prominent, centrally located bulge. The spiral arms are loosely wound, extending from the central region. A bar structure is present. The arms display a clumpy structure, suggestive of active star formation regions. The galaxy exhibits a moderate inclination relative to our line of sight, allowing for clear observation of the spiral structure. There is evidence of a possible minor disturbance or interaction, potentially a small tidal feature or asymmetry in the outer disk. Based on its color profile it is likely undergoing moderate amounts of star formation.
