The galaxy presents as a spiral galaxy with a prominent disk. The disk appears to be slightly inclined relative to our line of sight. Spiral arm structures are visible; however, they are somewhat diffuse. The central bulge seems moderate in size. There are no major morphological irregularities such as tidal tails, strong lopsidedness, or obvious signatures of a major merger event. The galaxy's overall color is bluish, suggesting ongoing star formation, although some regions of redder hues are also discernible, potentially indicating older stellar populations or dust obscuration. The galaxy exhibits a noticeable central concentration of light.
