The galaxy presents as a spiral, observed at a moderate inclination angle relative to our line of sight. Evident spiral arm structure is visible, exhibiting a somewhat patchy morphology. The arms appear relatively open, though tracing their full extent is challenging due to the image resolution. A central bulge is present, and the disk appears to be dominated by a brighter bulge component, indicating a larger central mass concentration. There is a hint of a bar-like structure extending through the central region. The overall color suggests active star formation, and/or a younger stellar population, particularly in the spiral arms, though this cannot be definitively determined from the image alone. There are hints of tidal disturbances, with some asymmetry visible in the arm structure, suggesting possible interactions with other galaxies.
