The object appears to be a spiral galaxy, oriented approximately face-on relative to our line of sight. The galaxy exhibits a well-defined disk structure with prominent spiral arms emanating from a central bulge. The spiral arms appear relatively tightly wound, displaying a medium pitch angle. Evidence suggests the presence of two main spiral arms. The central bulge appears moderately sized and luminous, with a somewhat elliptical shape. A bar structure seems present within the central region. The disk exhibits a relatively high degree of flatness, indicated by the axial ratio. There is some color variation visible within the spiral arms, suggesting active star formation regions. The overall morphology indicates this is a relatively massive galaxy with significant star formation activity. No major mergers appear to be occurring, but some minor disturbances could be present.
