The observed galaxy exhibits a predominantly disk-like morphology, though with some features indicating possible disturbances or interactions. The central bulge is visible but appears relatively small, suggesting a later type spiral or potentially a barred spiral galaxy. There appears to be a subtle bar feature spanning the central region. Faint and patchy spiral arm structures are discernible, though not sharply defined. Evidence of star forming regions is visible, particularly within the arms. Overall, the galaxy displays a complex structure that may be the result of past minor mergers.
