The galaxy presents as a spiral structure, observed at a near-edge-on inclination. Distinct spiral arms are discernible, although partially obscured by the viewing angle. The arms appear loosely wound, extending outwards from a central bulge. The bulge region displays a concentrated luminosity, exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. The disk of the galaxy presents a bluer tone compared to the bulge, which is indicative of ongoing star formation. A weak bar structure appears to be present within the central region. There is no evidence of any major merging events, though some minor disturbances cannot be ruled out due to the limited resolution. The overall morphology suggests a galaxy undergoing active, albeit moderate, star formation within its spiral arms.
