This galaxy presents as a spiral type, exhibiting a defined disk structure. The arms are prominent and well-resolved, demonstrating a multi-armed morphology, with hints of tight winding near the core and a more open structure further out. The central bulge appears relatively small. There is evidence of a bar-like structure crossing the center of the galaxy, though it seems somewhat weak or indistinct. Star forming regions are present within the arms. The overall appearance suggests a well-formed, though not entirely undisturbed, spiral galaxy, showing only minor signs of interaction or recent merger activity. The colors are indicative of a mix of stellar populations, with bluer regions associated with younger stars in the spiral arms, and yellower hues in the bulge indicating older populations.
