The object presents as a spiral galaxy at a redshift of approximately 0.101610. The galaxy exhibits a clear disk structure with prominent spiral arms. The arms appear tightly wound in some regions, and more open in others. A notable central bulge is present, contributing significantly to the overall luminosity of the galaxy. The bulge appears moderately sized. There may be a bar structure within the central region. The disk shows asymmetry suggesting possible interactions or internal disturbances. The galaxy's orientation is close to face-on. The color gradients suggest differential stellar populations within the galaxy, with bluer regions tracing areas of recent or ongoing star formation and redder regions indicating older stellar populations.
