The galaxy presents as a spiral galaxy, viewed at a moderately inclined angle. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. Prominent spiral arms extend outwards from the bulge, displaying a bluer color, which indicates the presence of younger, hotter stars and ongoing star formation within these regions. The arms appear somewhat flocculent, and patchy, with clear evidence of HII regions. The disk of the galaxy appears relatively thin and elongated, characteristic of a late-type spiral. Overall, the galaxy shows characteristics of a well-defined spiral structure with moderate star formation activity concentrated along the arms.
