The galaxy presents a morphology consistent with a spiral type. The galactic disc is observed at a moderate inclination. The bulge appears prominent, exhibiting a concentrated luminosity gradient toward the central region. Spiral arms are clearly discernible, though somewhat diffuse, displaying a multi-arm structure. The winding of these arms seems moderately tight. There's a possible bar-like feature extending through the central region, and the arms are seen to emerge from near the ends of this feature. Patches of blue color are distributed along the spiral arms, indicating ongoing star formation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions.
