The galaxy appears to be a spiral type, exhibiting distinct spiral arm structures. The arms are relatively well-defined and extend outwards from a central bulge. The winding of the spiral arms ranges from moderately tight to somewhat loose, with most arms tracing two primary paths. The central bulge appears to be of moderate size relative to the disk, appearing yellowish indicative of an older stellar population. There is strong evidence of a bar feature bisecting the galaxy's center, appearing prominent in the image. Star formation is actively occurring within the spiral arms. Overall, the galaxy's structure seems relatively undisturbed, with only slight hints of minor gravitational interactions with other objects. The galaxy is face-on and not edge-on.
